Текст
                    DEEP SKY ATLAS
Trion, Rappoport, Remaklus
Published by
Willmann-Bell, Inc.
P.O.Box 35025 • Richmond, VA 23235 USA
804-320-7016 • Fax (804) 272-5920
www.willbell.com
The Northern Hemisphere to -6°

Introduction This edition of Uranometria 2000.0 is a deep-sky atlas that plots more than 30,000 nonstellar objects and 280,035 stars to 9.75 magnitude on 220 double-pagc charts at a scale of 1.85 cm per degree of declination. In areas of heavy con- gestion close-up charts are provided al 2 or 3 times this scale with a stellar limiting magnitude approximating 11.0. While readers familiar with the first edition will see some similarities, many changes and improvements have been made, not only in the visual presentation, but in the underlying data from which it was created. To better under- stand our methodology, we present here a short history of modern astronomical cataloging. The modem era of cataloging began in 1958 with the completion of The National Geographic Society-Palomar Observatory Sky Survey [POSS] which was a photographic survey of the northern hemisphere night sky taken with the 48-inch Oschin Schmidt Telescope on Palomar Mountain. The southern hemisphere was photographed during 1975— 82 using the UK 1.2-meter Schmidt Telescope at Siding Spring Observatory in Australia. While both of these sur- veys extend beyond the celestial equator, only when com- bined do we have a high-quality photographic record from pole to pole. Until recently, catalogs based on these surveys were created by taking visual measurements from the photo- graphic plates, and compiling the data by hand. This meth- odology made these catalogs highly prone to human error, both in measurement and transcription. Moreover, subse- quent works look this earlier data at face value, thus propa- gating those errors through many years and many catalogs. If a newer catalog does make a legitimate correction, it may be deemed erroneous because it does not agree with the majority of other (incorrect) ones! Starting in the 1980s, both the POSS and the UK Schmidt Telescope Surveys were digitized (the photo- graphic plates were scanned and converted to computer files) by the Space Telescope Science Institute as part of an cight-year effort to support the Hubble Space Telescope. By the mid-1990s this data, now called the Digitized Sky Survey (DSS), and compressed by a ratio of 10:1, was available to the general public for download via the Inter- net. With the availability of the DSS to anyone with a com- puter and Internet access it was possible to obtain DSS images and verify catalog data against the original source—the sky itself! However, manually downloading and inspecting images from a very large list of objects would be a daunting task, and corrections would still have to be transcribed by hand—a process both time consuming This 1687 allegorical engraving from Johannes Hevclius’ Firmamentu Sobiescianum sive Uranographia depicts Urania the Muse of the Hea ens, with a stellar tiara and holding the Sun and Moon. She is su rounded by figures symbolizing the five bright planets. U.S. Nav Observatory, Washington. DC. and open to human error. What was needed was a way t more or less automate the process of inspecting DS; images and recording corrections. The solution to thi problem was provided by Emil Bonanno in the form of highly modified version of his commercial computer pro gram, Megastar: A Sky Atlas for Windows. Normally, Megastar allows a user to replace the pro gram's artificial sky with perfectly registered images fror the DSS, while at the same time displaying superimpose scaled symbols from the stellar and nonstellar deep-sk object databases. This allows a user not only to see the ret stars, galaxies, clusters, and nebulae, but also to see wher the various catalogs place them: an object's catalog posi tion, orientation and size can quickly be compared to th actual object recorded on film—and this same image ofte; is what the original cataloger used.
Bonnano’s custom program added tools to allow the manipulation of the nonstellar deep-sky object symbols: to move them, and to change their sizes and orientation (such as position angle for galaxies). For example, when a spe- cific nonstellar object’s catalog symbol did not fall pre- cisely on the DSS image, the symbol could be moved to make the match. The end result is that any changes made in an object's position, size, orientation, etc., were automati- cally transferred to the Uranometria 2000.0/Deep Sky Field Guide database. Deep-sky objects were selected for inclusion in this atlas using more clearly defined limits than was the case in the first edition. Galaxies were chosen based on an approx- imate magnitude cutoff of 15 or a major axis of at least 1.5 arcminutes, with occasional exceptions for objects that did not meet the criteria but which had some relationship to another object that did. An example would be a fainter or smaller galaxy superimposed on a larger one. However, all NGCs were included regardless of magnitude or size. In addition, all planetary nebulae known as of early 2000 have been included. All objects from a catalog of open clusters in the forthcoming book Star Clusters by Steven J. Hynes and Brent Archinal which were clearly visible on the DSS and likely to be visible with amateur instruments were selected. And new to this edition, all confirmable dark neb- ulae from Barnard's Atlas of Selected Regions of the Milky Way, Part II: Charts and Tables have been depicted. While everyone’s favorite “challenge object’’ may not have been included, what you have before you is a greatly expanded database, with a much higher degree of accuracy and util- ity, that should push the envelope for all observers. The Stellar Database In 1997 the European Space Agency [ESA] published the Hipparcos and Tycho Catalogues (ESA SP-1200), which provided highly accurate positions and magnitudes for about a million stars to ~11 magnitude. In 2000 ESA pub- lished the Tycho-2 Catalogue which increased the database to about 2.5 million stars. The Tycho-2 positions and mag- nitudes are based on the same observations as the Tycho-1 Catalogue collected by the star mapper of the ESA Hippar- cos satellite, but Tycho-2 is much bigger and slightly more precise because it used a more advanced reduction tech- nique. To a very close approximation the Hipparcos/Tycho magnitudes match “true” visual (V) magnitudes. This atlas plots 280,035 of these stars to 9.75 magnitude on the 220 double-page charts and to ~11.0 on the 26 “close-up” charts. Three data sources were used for determining the variability of stars. The Variability Annex of the Hipparcos Catalogue was the reference for over half of the stars of this type. The second source was the variability flag in the Tycho Catalogue, which accounts for about 43% of these classifications. Only those Tycho stars which were flagged as having “strong evidence for variability” were classified as variable. The third source was the General Catalogue of Variable Stars [GCVS] (Kholopov, et al., 1998). The Tycho data was correlated with the GCVS, using a combi- nation of positional and magnitude criteria. This resulted in about 6% of the variable star classifications. Preference was given to the Hipparcos data for assign- ing minimum and maximum magnitudes, since these val- ues are presumably more reliable than Tycho’s. For the variable star names, the majority came from the cross-ref- erence information in the Hipparcos Variability Annex. This was found to be somewhat incomplete, however, and an additional 944 variable names were obtained through correlation with the GCVS. Uranometria 2000.0 is not intended to be a compre- hensive atlas of variable stars, even though more than 6,300 of them are plotted and labeled. The serious variable star observer will encounter omissions. The primary reason for an omission is attributable to the scale of this atlas. Denoting variables in areas densely populated by deep-sky objects, or in rich star clusters, would have introduced excessive clutter on the chart. However, no variable star of “significance” was knowingly omitted for this reason. Most will be found to have a relatively small amplitude (less than 0.2 magnitude), or to reside at the faint end of Uranometria’s magnitude limit. Our main concern was that we plot those variables which have a large brightness range and a relatively bright maximum to reduce the possibility that an “unexpected” star will alter the star pattern that the observer is using to locate a faint deep sky object. For example, a star may spend most of its time at 12th magnitude, and then brighten to 7th. An observer who is unaware of the location of such a star may be confused by the new star pattern which this would then present. It is this situation which we have attempted to avoid. Alternatively, a variable star with a maximum that is near the faint limit of this atlas may decrease in brightness by several magnitudes. In this case, there would be a star missing from the expected pattern. Nominally, the variable star symbol provides a qualitative representation of the minimum and maximum brightness of the star. But for stars whose maximum is 8th magnitude or fainter, the small size of the symbol prevents accurately displaying the star’s minimum brightness. In an extreme case, a plotted variable star may decrease to 14th magnitude or fainter. The user should keep this in mind when star-hopping a field containing moderately faint variables. In order to maintain consistency in Uranometria 2000.0, the minima and maxima of variables has been taken from the Tycho and Hipparcos data whenever possi- ble. We would expect that variable star observers will have other sources for this data, and there will no doubt be dis- crepancies. Compared to most well-studied variable stars, the number of observations made during the Hipparcos mission was relatively small. Therefore this data may not reflect the true extremes of a given star’s magnitude range. Double star classification was based upon both the Hipparcos and Tycho Catalogues. The former contains sev- eral indicators of duplicity: “Number of Components,” “Doublc/Multiple Systems Annex Flag,” “CCDM Identi- fier,” and “Component Identifiers.” All of these were taken 2
into consideration in the double star classification process. For objects not contained in Hipparcos, the classification process was a bit more difficult. The Tycho Catalogue “resolves” many double stars, giving each component a separate entry. While there is a “duplicity flag” in the Tycho Catalogue, it only identifies those entries which are unresolved. Identification of wider doubles had to be inferred from other information, such as the “Proximity Flag” and “CCDM Identifier.” This was supplemented by searching the data for pairs of stars with separations of less than 60 arcseconds. From this information, additional dou- ble star assignments were made. With the exception of these doubles, all of the angular separation and position angle data in Uranometria 2000.0 came from Hipparcos. Arrangement of Charts and Labeling This atlas is composed of 220 charts spanning two vol- umes: Volume 1, The Northern Hemisphere to -6° and Volume 2, The Southern Hemisphere to +6°. Also included are 26 additional 2x and 3x close-up charts covering con- gested areas. A third volume, Deep Sky Field Guide (DSFG), provides valuable data tailored to the observer’s needs, in a condensed form for each chart. This atlas uses the International Celestial Reference System and the grid is in 2000.0 coordinates measured from the Celestial Equator and Equinox at the beginning of the year 2000. The epoch of the positions is that of the Hip- parcos and Tycho Catalogues (J 1991.25) which, consider- ing the scale of this atlas, is undetectable for all but a very few stars between that date and 2000.0. Constellation boundaries are based upon those of E. Delporte and endorsed, in 1930, by the International Astro- nomical Union {Report of Commission 3). Precession since then accounts for their no longer being aligned with the great circles of Right Ascension (R.A.) and circles of Dec- lination (Dec). Constellation names are placed near a bor- der for easy identification. The scale of the main atlas is 1.85 cm = 1° of declina- tion. Stars are drawn as filled circles, their relative size determined by their visual brightness in a smooth taper between 0.0 and 9.7 magnitude. The stellar taper for the close-up maps is 2.0 to 11.5 magnitude. Stars having proper names are so labeled (Castor, Polaris, etc.). The brighter stars are labeled by Flamsteed number and Bayer letter (if one exists). Double or multiple stars with separa- tions less than Г are indicated by a line protruding from opposite sides of standard-sized dots, with the dot size based on integrated magnitude. For separations greater than 1' the components are plotted independently. Variable stars are denoted by a concentric circle-and- dot symbol. The outer circle shows the star’s maximum brightness. The Ecliptic is drawn as a dashed line, labeled (once per chart) “Ecliptic,” and calibrated each Г in longitude. The Galactic Equator is shown with a dashed-dotted line, labeled (once per chart) “Galactic Equator,” calibrated each 1° in longitude. Also labeled are the North and South Galactic Poles and the North and South Ecliptic Poles. In general, deep-sky objects are labeled by NGC num- ber (without prefix, i.e., 7331) or 1C number (with prefix “I”, I 4567); for the Messier catalog, by a number precedec by an “M,” M103. Deep-sky objects may also be labeled bj popular names. Objects taken from other works generally are identified by the name of the catalog or an abbreviatior of its author’s name. To reduce congestion on the charts, we have chosen tc abbreviate prefixes and remove leading zeros as follows: CGCG = С (C 4-61) ESO = E (E 30-10) MCG = M (M-1-22-26) PN G = P(P 5.2-18.6) UGC = U (U 7580). The Close-up Charts In areas of particularly heavy congestion a shaded rectan- gular box outlines the boundaries of a 2x or 3x close-up chart. These rectangles are labeled with an “A” followed by a number. Charts with these numbers appear following the main charts. In some of the most crowded areas of close-up map rectangles found on the main charts, you will notice thal the symbols of some objects have been filled with gre> shading and are without labels. These objects are identifiec on the close-up maps. Navigational Aids Getting around a large-scale atlas can be a daunting task To make this atlas more user-friendly a number of naviga- tional aids have been added to it. Immediately inside the front cover you will see four large-scale finder charts thal are keyed to both chart numbers, and the tabbed declina- tion bands marked on the outside edge of each right-hand page. Also at the front, immediately following the findei charts, is a table that lists the map closest to the mean cen- ter of each constellation along with other “top line” infor- mation about the constellations. Next, you will find a 22- map, 6.5-magnitude star atlas keyed to the Uranometria 2000 charts. These maps provide an intermediate step between the main charts and the finder charts found just inside the front cover. Turning to the main charts, you will find directions tc contiguous ones in the form of arrows around the edges ol each chart. The legend on the right-hand page of each includes its R.A. and Dec range along with the names of up to four constellations appearing on it, in order of decreas- ing area. Finally, there is a scries of Indexes at the back of the book that cross-references star names, Bayer letters, com- mon names, Messier objects and NGC/1C designations. Ir the companion DSFG the complete nonstellar object list is indexed by chart and DSFG table number. All these Indexes are keyed to objects within the R.A. and Dec 3
boundaries of a given map. Occasionally, objects just out- side a chart’s boundaries are plotted to alert the user that something interesting is just “next door.” Where this hap- pens the Index entry is for only the adjacent chart, on which the object falls within its boundaries. The Nonstellar Database Galaxies Uranometria 2000.0 plots 25,895 galaxies. They are shown as open ovals, with objects larger than 5' drawn to scale. Galaxies with a major axis less than 5' are binned into one of three groups, using symbols to represent the following size ranges: 5-2', 2'-!', and less than 1'. On the 2x close-up maps, galaxies larger than 2.5' are plotted to scale, and those smaller than 2.5' are binned as follows: 2.5-Г, T-0.5', and smaller than 0.5'. On the 3x close-up maps, if larger than 1.7' they are plotted to scale while those that are 1.7' or smaller are binned as follows: 1.7'- 0.6'. О.б'-О.З', and less than 0.3'. For all galaxies other than those that have equal major and minor axes, the symbol is oriented on the chart in the direction of the major axis. Most galaxies have been listed in more than one of the “standard” catalogs. In this work we have adopted the fol- lowing labeling precedence: New General Catalogue (NGC), Index Catalogue (IC) Uppsala General Catalogue (UGC), European Southern Observatory (ESO), Morpho- logical Catalogue of Galaxies (MCG), Catalogue of Gal- axies and Clusters of Galaxies (CGCG ), and Catalogue of Principal Galaxies (PGC). Galaxies are complete star systems. A typical one is composed of billions of stars, while the largest can easily exceed a trillion stars. For the most part, clusters and nebu- lae in other galaxies are well out of visual range. Amateurs equipped with large scopes will be able to observe detail in only a few hundred of the brightest examples. For this work galaxies were selected that have a В magnitude of 15 or brighter, or a major axis of 1.5 arc- minutes or larger. As noted before, all NGC objects are included regardless of magnitude or size. Positions, dimen- sions, and position angles were confirmed, or modified where necessary, by visual inspection using Digitized Sky Survey images. There are undoubtedly still some identifi- cation and positional problems in the resulting galaxy data- base, but we believe that the procedures we have followed have greatly reduced their number. Position angles (PA) are given for noticeably elon- gated galaxies and were obtained directly from a visual inspection of the DSS. Obviously, position angles do not apply to circular objects. These angles, expressed in degrees, are measured from north through east. A value of 0° implies a north-south elongation. A PA of 90° indicates an east-west elongation. After a further quarter-turn coun- terclockwise, the object is oriented in a PA of 180° (equiva- lent to 0°), again in a north-south direction. All PAs for galaxies are referred to the first half of the circle, so they do not exceed 179°. To measure the PA of a galaxy in your eyepiece, you must first determine north as precisely as possible. The best method of doing so, especially for telescopes on altaz- imuth mounts (Dobsonians, etc.), is to first determine west. This is easily done by centering a bright star in the eye- piece and removing all drives to the telescope so that the star drifts to the edge of the field. The point where the star exits the field is west. North will then be 90° counterclock- wise from the west point (clockwise for refractors and Schmidt-Cassegrain telescopes with star diagonals). Knowing the position angle of a galaxy with respect to others can obviously be very helpful in identifying it in a crowded field. In a similar way, determining the PA of elongation for an “unknown” galaxy aids in identifying it later through catalog descriptions or on sky survey photo- graphs. Galaxy Clusters This atlas contains 671 galaxy clusters derived from George Abell’s 1958 catalog based upon photographs from Mt. Palomar Observatory. In 1980 Abell issued a revision to this catalog, and in 1984 he died while engaged on a southern extension of it using photographs taken at the Anglo-Australian observatory. This work was expanded upon and subsequently completed in 1989 by Harold Cor- win and Ronald Olowin. Objects from the 1958 catalog are designated herein with an “A,” while those from the 1989 extension bear an “AS” prefix. Diameters for “A” objects are taken directly from Abell’s revised catalog. Similar data was not available for the “AS” clusters so the diameters were estimated based upon the distance class. For all “A” objects having the same distance class, mean diameters were computed, and those values were applied to the “AS” clusters. Therefore, these dimensions are indicative only, not precisely mea- sured. Until the advent of very large amateur telescopes and CCD imaging these objects were well beyond the reach of the amateur community. Open Clusters This atlas plots 1,617 open clusters, including those in the Magellanic Clouds. They are shown as dotted open circles, with objects larger than 5' drawn to scale on the main charts. True open clusters are relatively young objects scat- tered throughout the disk of the Galaxy. A familiar exam- ple is the Pleiades, found on Chart 78. These objects are also known as Galactic clusters, since all but those nearest the Earth are found near the plane of our Galaxy (Chart 8 shows twenty-seven). Over time many objects cataloged as clusters have been proven to be just chance groupings or apparent groupings of unrelated stars. Many of these objects have NGC or IC designations and are well estab- lished in the literature. We have chosen to include them as clusters here. The companion DSFG provides specifics. 4
In the very youngest cases, the remnants of the gas from which they formed are visible as nebulae in the sur- rounding field. In fact, a small number (78) of open clus- ters share a single designation with their nebulae. An example is IC 1396 on Chart 19, which is listed as both an open cluster and a bright nebula in the respective sections, has two separate symbols on the chart, and is listed twice in the Index. The number of stars in these objects ranges from only a few to thousands. In appearance they vary from rich, compact, easily distinguished objects, to a few stars so loosely grouped that they are hardly discernible from the surrounding star field. Many of the latter require experi- mentation with different apertures and magnifications to be seen. Small telescope users will probably be able to view a larger percentage of open clusters than other types of deep- sky objects. The principal source used for data on these objects is the book Star Clusters by Brent Archinal and Steven Hynes, in press, to be published by Willmann-BelL This atlas uses a subset of that data which was selected by a review of the entire catalog by direct inspection of the DSS images by DSFG co-author, Murray Cragin. His criteria were general visibility and the likelihood that the object could be seen by amateurs. Globular Clusters Some 170 globular clusters, including both Milky Way and Magellanic Cloud objects; are contained in this atlas. They are shown as a continuous-line open circle with an internal cross. On the main charts globulars larger than 5' are drawn to scale; on the 2x close-up maps they are to scale if their diameter is larger than 2.5', and on the 3x maps, if they are larger than 1.7'. While open clusters have irregular outlines, globulars are strongly circular, and their stars are much more numer- ous, and densely packed toward the center. They are among the oldest objects to be found in galaxies, with ages near 13 billion years. The number of stars comprising them can range from 10,000 to over 100,000. While open clusters are found strictly in the Galactic plane, globulars are grouped into two regions: around the “hub” at the center of our Milky Way and in its extended Galactic halo. All are gravitationally bound to our Galaxy even though a few are twice as far from its center as the Magellanic Clouds! Globulars are most numerous in the direction of the Galac- tic center (Chart 146 shows 22 of them), although many of these are greatly dimmed by interstellar dust (the non-NGC globulars listed for Chart 145 are examples). Star Clouds We have chosen to plot 14 star clouds. These objects are composed of countless stars and often span vast stretches of the night sky. When viewed at low power the nebulosity is often overlaid with sparkling stars which often do not show up in photographs. Usually star clouds are so vast that they cannot be plotted on a large-scale atlas however Chart 164 plots 7: NGC 6360. 6415, 6421, 6437, 6455, 6476 and 6480. Another, M 24 on Chart 145 is a visually striking star cloud that contains a number of other observ- able objects. Because there are so few of these plotted objects wc have not included them in the legend but have assigned a special symbol and annotated the name with “(star cloud)” to aid in their identification. The symbol siz- ing is the same as that used for open clusters. Bright Nebulae We draw to scale 377 bright nebulae with a solid outline if larger than 1 O'. Objects smaller than 10' are drawn as solid- line square boxes in two sizes (10' to 5' and less than 5'). On the 2x close-up maps they are plotted to scale if larger than 2.5'; on the 3x maps, if larger than 1.7'. These objects, also called diffuse or Galactic nebulae, occur in two main classes depending on their source of illumination: emission and reflection, although they occa- sionally are a combination of the two. Much less common is a third type of bright nebula, the supernova remnant (SNR). Emission nebulae are clouds of dust and glowing hydrogen gas, sometimes referred to as H II (“H-two”) regions. The atoms in the cloud are ionized by nearby hot stars, and when the excited electrons fall back to their pre- vious energy state, the process releases energy in the form of visible light. A well-known example is the Lagoon Neb- ula, found on Charts 145 and 146. Since most of the light visible from emission objects comes from just the three lines produced by hydrogen (H[3 at 4861 A) and oxygen ([OIII] at 5007A and 4959A), the use of narrow band “neb- ula” filters can be helpful in viewing them. Reflection nebulae have the same composition as emission objects but lack stars sufficiently hot to cause the gas comprising them to fluoresce; therefore, they shine merely by the dust in the nebulae scattering starlight (the gas docs not actually reflect any light). Good examples are the nebulosities surrounding the Pleiades star cluster (Chart 78) and M78 in Orion (Chart 116). Because these objects scatter starlight of all colors, filters are not gener- ally helpful in viewing them. A supernova remnant is the remains of a catastrophic stellar explosion, wherein much of a star’s material is ejected, often as a highly-structured cloud. Examples are the Veil Nebula in Cygnus (Chart 47) and the Crab Nebula (Ml) in Taurus (Chart 77). These objects have strong emis- sion lines similar to H II regions, hence also benefit from the application of nebula filters. Dark Nebulae This atlas contains 367 dark nebulae, which arc drawn to scale with a dashed outline if larger than 10'. Objects smaller than 10' are drawn as dashed-line square boxes in two sizes (10' to 5' and less than 5'). On the 2x close-up 5
maps they are plotted to scale if larger than 2.5', on the 3x maps, if larger than 1.7'. Dark nebulae are composed of clouds of dust and gas sufficiently dense as to become opaque. They are detect- able if positioned between the observer and a bright nebula or a very dense star field, against which they can be seen silhouetted. Observationally, dark nebulae are among the most difficult deep-sky objects. The Coalsack, near the Southern Cross (Charts 198 and 209), is an example clearly visible to the unaided eye because it happens to lie in front of the rich, starry background of the Milky Way. On the other hand, the well-known Horsehead Nebula (cataloged as Barnard 33 on Chart 116) is much more typical. Il is a difficult object because of its small size and because it lies in front of a rather faint background object, emission neb- ula IC 434. In this case the resulting contrast between the dark nebula and background is very low, making it difficult to distinguish. Dark nebulae are usually seen best with wide-field, low-power eyepieces, which provide a large, bright surrounding field. While these objects emit no light of their own, nebula filters may help increase the contrast if the background is an emission nebula. Planetary Nebulae 1,144 planetary nebulae are plotted, shown as open circles with four protruding lines, in four sizes representing the following categories: those having diameters greater than 30", 30" to 10", 10" to 5" and less than 5". On the close-up charts two additional symbols are used: greater than 60" and 60" to 30". Planetary nebulae are shells of gas thrown off by stars having approximately the Sun’s mass, that are nearing the end of their evolutionary cycle following the red-giant stage. The shell gradually expands, until after perhaps 1 ()().()()() years it becomes undetectably thin and all that remains is the central star. Some of the earliest such objects discovered (e.g., NGC 3242 on Chart 151, and NGC 6210 on Chart 68) were found by William Herschel, who noted the resemblance of their well-defined disks to those of planets, and gave them the name “planetary nebulae”, but of course they have nothing to do with planets. The brightest planetaries have a substantial disk, typi- cally 30 arcseconds across, but the majority listed here are stellar (or nearly so) and can be identified at the eyepiece only with a nebula filter or direct-vision prism. Chart 164 lists over 100 such objects, hardly any of which are larger than a few arcseconds in diameter. A few of the oldest and nearest examples are so distended as to be practically invis- ible against the background sky. Between these two extremes are planetaries that come in about as many shapes as there are objects, including the aptly-named Ring Neb- ula on Chart 49 and the complex southern object NGC 5189 on Chart 208. Invisible light, planetary nebulae shine predominantly at the two wavelengths emitted by doubly-ionized oxygen, denoted by the symbol [ОШ]. Typically, 90% of the visu- The Greek Alphabet Alpha a Iota i Rho P Bela p Kappa к Sigma О Gamma Y 1 .ambda X Tau T Delta 8 Mu M IJpsi Ion X) Epsilon e Nu V Phi Ф Zeta c Xi Chi X Eta n Omicron 0 Psi V Theta 0 Pi Л Omega (1) ally-detectable light comes from the [OIII] lines at 5007A and 4959A in the blue-green part of the spectrum. As a result, when an [OIII] filter is placed between the eye and the eyepiece, stars are dimmed by as much as three magni- tudes (the night-sky light even more), while light from a planetary passes through virtually unchanged. By rapidly passing an [OIII] filter between the eye and eyepiece and out again while examining the field, a planetary will usu- ally appear to “blink” as the stars are dimmed, and the neb- ula maintains its brightness. There are a few planetaries that have weak [OIII] emission (a bright example is PN G64.7+5.0, Campbell’s Hydrogen Star, on Chart 48), and these are best viewed either directly or with an Hp filter, which passes the line that is brightest in these cases. Radio Sources These objects are shown as open triangles when the source is invisible or below the chart’s limit. There are about 260 of them plotted in this atlas. About 100 additional sources are both radio and quasi-stellar objects or x-ray emitters. Where the visible source is plotted, as in the case of a bright star (e.g. 5 Cas) or a galaxy, the special symbol does not appear. In order of preference they are identified by their designation from the Third Cambridge Catalogue of Radio Sources (3C), the 4C number and then PKS without prefix formed by concatenating the hours and minutes of R.A. with declination truncated to tenths of a degree. X-Ray Sources These are shown with an open centered “X” in cases where the source is invisible or below the chart’s limit. About 35 of them are included herein. Where the visible source is plotted, the special symbol does not appear. Objects are generally labeled by common name (e.g. M82, NGC 1815, LMC S-2 [Large Magellanic Cloud], or у Cas). Quasars Quasars (Quasi-stellar objects) are identified by open cir- cles with superimposed diagonal line. In order of prefer- ence they are labeled with: 3C number, 4C number, and then coordinate designations as established in Sky Cata- logue 2000.0, Volume 2 by concatenating the hours and minutes of R.A. with declination truncated to tenths of a degree. 6
LYNX AURIGA URSA MAJOR CANES VENATICI CAMELOPARDALIS URSA MINOR PERSEUS CEPHEUS BOOTES DRACO TRIANGULUM CASSIOPEIA LACERTA ARIES HERCULES ANDROMEDA LYRA CYGNUS PISCES VULPECULA PEGASUS OPHIUCHUS SAGITTA AQUILA DELPHINUS EQUULEUS 103 CETUS SERPENS CAUDA SCUTUM AQUARIUS SAGITTARIUS CAPRICORNUS SCULPTOR SCO PISCIS AUSTRINUS MICROSCOPIUM CORONA BOREALIS Oh 23h 22h 21h 20h 19h 18h URANOMETRIA 2000.0 - INDEX -1.5 -10 -OS Stellar Magnitudes (V) 0.0 0.5 1.0 1.5 2.0 2 5 10 15 4.0 4.5 5.0 5.5 Cupynyhlf 1987 2001 Wtflmann-h’U. IM Гmi / Лату Ла/трлрап Wilt Remaklm
Index N2 — Volume I — 18h to 12h AURIGA CASSIOPEIA ANDROMEDA CAMELOPARDALIS LACERTA LYNX CEPHEUS URSA MAJOR CNC CYGNUS DRACO MINOR VULPECULA LYRA SAGITTA AQUILA CORONA BOREALIS COMA\ BERENICES HERCULES BOOTES SCUTUM VIRGO 109 108 OPHIUCHUS CRATER CORVUS SAGITTARIUS LIBRA HYDRA SCORPIUS CEN SERPENS CAUDA SERPENS CAPUT URSA MINOR CANES VENATICI 16h 15h 13h 12h URANOMETRIA 2000.0 - INDEX Stellar Magnitudes (V) 2 0 2.5 3.0 3 5 4.0 4 5 5.0 5.5 1 0 0 5 0.0 Copyrrani /987-200/ Mf/marin-fle/C ft/i Wk Гт? Bariy fapiwrf ' Will Яетайля
Index N3 — Volume I — 12h to 6h ANDROMEDA CEPHEUS HERCULES DRACO CASSIOPEIA CAMELOPARDALIS PERSEUS BOOTES AURIGA TAURUS LYNX MINOR ORION GEMINI CANCER VIRGO SEXTANS MONOCEROS CORVUS HYDRA LEPUS CRATER PUPPIS CANIS MA|OR PYXIS COLUMBA HYDRA ANTILA CANES VENATICI CORONA BOREALIS COMA BERENICES URSA MINOR CANIS MINOR URSA MAJOR 12h 11h 1Oh 7h 6h Stellar Magnitudes (V) URANOMETRIA 2000.0 - INDEX -1.5 -1.0 0.5 0.0 0.5 1 0 1 5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5 5 CopyrtghlC 198/ 2001 WHImonn-MI. Inc
Index N4 — Volume I — 6h to 0h CVN HERCULES DRACO LYRA URSA MINOR URSA MAJOR MINOR CYGNUS LYNX CAMELOPARDALIS CNC CASSIOPEIA < LACERTA GEMINI AURIGA PEGASUS ANDROMEDA PERSEUS TRIANGULUM ARIES TAURUS PISCES ORION MONOCEROS AQUARIUS CETUS LEPUS ERIDANUS FORNAX COLUMBA SCULPTOR CAELUM CANIS MAJOR Oh 6h 5h URANOMETRIA 2000.0 - INDEX Stellar Magnitudes (V) •1.5 -1.0 -0.5 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 Copyright © 1987-2001 WHImunn Bell, inc
4Zl </Г/ CAMELOPARDALIS A? V8264 U8454 URSA MINOR U86 5 U10263 2300 CEPHEUS / U10740 1544 V406 DRACO U 285 3C61.1 U 198 3C435.1 RU AR 88 0]h +84 .5 2 a О U4396 'U4601 У ° U4100 U3992 • . U3993 0 1.469 U4297 о 1.499 O'- U4348 M+14-4-49 V411 2268 О 1.455 о 2276 P M+15-1-12 U3528 U3522& U3500 : о U3654 V410 о • U3715 М+14-4-29 ° ®OV О U5083A U3536A U3442 °; U3336 ° CAMELOPARDALIS CEPHEUS OW25/ U3253\Q M+14-2-9 U1039 . URSA MINOR o.o dndbnqhter 0.5 1.0 1.5 2.0 25 3 0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 80 8.5 9.0 9.5 9.7 3172 Polarissima Borealis North Celestial Pole Polaris 4 a +85° +90° +89 +88 +87 &V377 ©V378 +86° 00h U11267 U10923 о 24 Ф23 3 CEPHEUS Variable Stars О ® ®> (f) ® ® @(S) ® (•)(•) о Amplitude Amplitude Amplitude Amplitude 1 0 mag or less 2.0 mag. 3.0 mag. 4 0 mag. П Nova Q Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Individual members are plotted if separation exceeds 60' Copyright О 1987-2001 Willmann-fteil, Inc
CAMELOPARDALIS О 2300 P 2276 U4297 о U3654 U8264 . U8454 URSA MINOR U8615 CEPHEUS / 24 U1285 3C61.1 U 98 3C435. RU AR M+14-2-9 f85° O]h +84° ’ 1544 Struve s Lost Nebula M+14-4-29 ® OV ©V378 0 о ' U4601 1.512 1.499 . o'- U4348 M+14-4-49 о • U3715 U3536A Open Star Clusters and Asterisms to scale V411 U1039 Globular Star Clusters to scale U10263 US 08 ЗА URSA MINOR Planetary Nebulae M+15-1-12 3172 oW О Polarissimo Borealis North Celestial Pole Polaris 1 (X • 188 >30' 30H-10' 10'-5r <$' +90° +8?: +88_ +87 00h ФУ377 Bright & Dark Nebulae to scale 10'-S’ [J • <S' Galaxies >5 Io scale 2 1 < major axis U11267 U10740 о U10923 DRACO CEPHEUS ‘ Galaxy Cluster Io scale 00h00m to 24h00m +90° to +84° CEP UMI, CAM, DRA Wii Г1ГКУ1 / Barry'Rappoport / WtH Remakiui
2 лид brighter 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 О @ ® @ ® ® (•) ® ® (•) ® о Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4 0 mag Nova Q Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Individual members are plotted И separation exceeds 60" Copyright © 198/-200) Willmunn-Bell, Inc.
Open Star Clusters and Asterisms О О О to scale < 5' Globular Star Clusters ф ® Ф to scale < 5' Planetary Nebulae >30" 30"-10" 10" 5" <5" Bright & Dark Nebulae °::: to scale 10 -5’ <5‘ Galaxies >5' 5'2' 2'1' <V to scale major axis Galaxy Cluster ' “ X ; j to scale 02h20m to 21h40m +85° to +73° CEP CAS VW Tirion / Barry ftappaport / Will Kemoklui
3 0.0 anabnghier 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8 5 9.0 9 5 9 7 S © © @ © © (•) © ® © ® © Amplitude Amplitude Amplitude Amplitude 1.0 mag or less 2.0 mag. 3.0 mag. 4.0 mag к Nova 0 Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Individual members are plotted if separation exceeds 60” Cupynyht © 198/-2001 Willmann-Bell, Inc.
Open Star Clusters and Asterisms ' ' CJ) ’ to scale < 5‘ Globular Star Clusters ф Ф e to scale < 5' Planetary Nebulae Ф <- -Ф- Ф >30* 30"-10* 10"-5" <5M Bright & Dark Nebulae <C?c? □ □ □ о to scale 10' - S' < 5' Ga A >5' to scale laxies ООО 5-2 2-Г <Г major axis Galaxy Cluster •ч \ to scale 17h40m to 22h20m +85° to +73° DRA CEP, UMI Wil Ппол / Barry Ruppapurt I Will IternoHus
4 о U10471 u10447 U10446 M+13-12-3 .uw 06217 U10509 U10466 UrSA MINOR U10280 О о U10237 0 U10212 to '<%> URSA MINOR U10368 • (jy -~-L_DRACO lehjQm 16h20m --- +73° 16h00m и Nova Q Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Variable Stars © @ ® © © ® (•) ® ® (•) ® о Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2 0 mag 3.0 mag. 4.0 mag. Individual members are plotted if separation exceeds 60’ Mxibnghtw 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Cupynght © 198/-2001 Willmann-tell, Inc.
Open Star Clusters and Asterisms OO 0 to scale < 5' Globular Star Clusters Ф ® ® to scale < S' Planetary Nebulae -ф- -Ф- -Ф- ♦ >30” 30"-10“ 10'-5" <5" Bright & Dark Nebulae □ IJ D i-i to scale 10'-S' <5‘ Ga ^0 >5' to scale laxies о о о S'-2‘ 2-Г <1* mpjor axis Galaxy Cluster ( \ to scale 13h40m to 18h20m +85° to +73° UMI DRA, CAM VW Tirion / Barry Rappoport / Will Remakkis
5 12b Op 13h 1-3568 ^8148 07089 Ry 4127o '4P M+12-12-7’ ^2^4Qm 3C268.1 u2908 /А7500 ЗЬ^ 4589 4S/2' 07189 0 ° 4133 (j8!64 U8287 "8,83 U799S 49S4 и ^7872 “8120 Us^64 / 07097 ° CO J • ° 9 U7086 M+13-9-21 CAMELOPARDALIS 4331q 4189 о 4386 о 4319(^4291 M+13-9-23 07226 M+,8-9-3) о ’ о U80S2 4363 ♦ 4648 U7767 О AS 12h20m 12h00 Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. Q A X Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Nova Quasar Radio Source X-Ray Source 0 0 Individual members are plotted andbnghtw 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 if separation exceeds 60’ Copyttghl © 1987-2001 Willtnunn Bell. Inc
5 Open Star Clusters and Asterisms О О о to scale < S' Globular Star Clusters to scale < S’ Planetary Nebulae -ф- <> -Ф- < >30' 30"-10" 10"-5" <5’ Bright & Dark Nebulae <2?C? □ □ □ ::: to scale 10 -5' <5* Ga A >5' to scale laxies О о о S -2 2'-Г < r major axis Galaxy Cluster ; 'i to scale 09h40m to 14h20m +85’ to +73’ DRA CAM, UMI WH Гюм / Валу Rappoport I Will RemMus
6 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Variable Stars «Be® © ® © (•) ® Amplitude Amplitude Amplitude Amplitude 1.0 mag or less 2.0 mag 3.0 mag. 4.0 mag Nova Q Quasar A Radio Source x X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Individual members are plotted if separation exceeds 60’ Copyright© 1987-2001 Willmann-Bell, Inc.
07ъ +84° +83° ^0729+818 +81° +78° +77’ +76’ +75’ +82° У А U3929 to I.481 S\3 U4066 —с— (S) FH EV US»»6 U3636 0 ®с^ 2314°' • 08h +85° ~ CEPHEUS У3993 I- - U3992 0 2268 +80 +79° +74’ \ ° (Ч< \- о FF U3668 д 3C784J 2336 О I.467 U3794 • Ч U3675 и4057ъ ьо U4028 и4014 U3906* ‘ .EV "^Ги3717 < °vs» °й 2186 с> о* о U4080 о . U4041 о U3972 U3909 U3859 : С) U3858 и!”’° ЩТ05 (7ЪОО^ +73° — 08h00m • 2441 07h40m Open Star Clusters and Asterisms to scale < 5’ Globular Star Clusters to scale < 5* Planetary Nebulae -ф- <> < + >30" 30"-10" 10*-5" <5" Bright & Dark Nebulae D □ °: to scale 10'-S’ <5' 6г Ai >$' to scale laxies О о о S -2' 2' Г < Г major axis Galaxy Cluster \ 'i to scale 05h40m to 10h20m +85° to +73° CAM DRA, CEP, UMA Wil Tinon ! Barry Rappoport i Will Remoklui
+8Z +8: % +8. +8 +8 ^7o Osh о. V407° DI +7! +71 AN C7 04h40m Osh2o'm °5Ь10ъ 4? V408 • 4 •W09 00 and brighter 0.5 45(>S W/J7 о ^41 "5144 ^150 □ Individual members are plotted 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6 0 6.5 7.0 7.5 8 0 8.5 9 0 9.5 9.7 I if separation exceeds 60' U3057 . О 0 1-3S/ ° X 1530 04h +8 P U2896 U2907 • • •— U2906 0 1S73^+12^ Amplitude Amplitude 10 mag or less 2.0 mag. Amplitude 3.0 mag. CAMELOPARDALIS 04h20m 04h00m Amplitude 4.0 mag Q Д X Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Nova Quasar Radio Source X-Ray Source 1.0 Copynghte 1987-2001 Willrnann-Bell. Inc.
Open Star Clusters and Asterisms OO О to scale < S' Globular Star Clusters ф Ф ® to scale < S' Planetary Nebulae -ф- ❖ >30" 30"-10" 10"-S" <5" Bright & Dark Nebulae <2?C? □ □ о о to scale 10'-S' <S* Ga ^0 >S' to scale laxies Ooo S-2' 2-Г <Г major axis Galaxy Cluster О to scale 01h40m to 06h20m +85° to +73° CAM CEP, CAS Wil Tinon / Валу Rappoport / WiH Remokkts
8 ЛР'гОт 0.0 and bight* 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8 5 9.0 9.5 9 7 • ® (•) ® ® ® ° Amplitude Amplitude Amplitude Amplitude 1 0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. a Nova Q Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Individual members are plotted it separation exceeds 60’ Copynqhl CH 98 / 2001 WiHmann Belt. Inc
• CEPHEUS +73° +72° +71° +70° s +69° XY- +68° +66°. A° й *14 3C468. • О +64 VA?,6' +63° King 21 DD С .Us' \J8O&^ V375 o------ Ti6(V566) <StJ7 VAN Co^ 00h00m 23h52m +74° --------n--- • 7822 8e59 +67° +65° Ced2]4 Be 99 ,0° King 11 V461 \J457 7762 CASSIOPEIA +62’ — oohoom 23h52m V460 Pl 12.5+4 3.0 V816 .XX ’Be 101 Be 100.... \j8Uo ® \/3^7 <bufo^ 23h44m 23h36m 2}h28m A ,61° Open Star Clusters and Asterisms Globular Star Clusters Planetary Nebulae О О о e -ф- -ф- < +• to scale < 5' to scale < 5' >30’ 30"-10" 1О'-5и <5* to scale 10-5' Bright & Dark Nebulae □ Galaxies io scale major axis Galaxy Cluster to scale 01h20m to 22h40m +74° to +62° CEP CAS Wrf firiorr / Burry /tappuport / WJT Kemakkn
9 +73° +72’ ^6 о EK +69' +66’ 7142 +65° 22h48m +63° CEPHEUS 22h00m 21h52m (V337)@ ?2h24m 22h^ °8 21^52m 21h44m 21h36m +74’ ®DM ® V445 16 (71/861 * 0 U11818- .VZ -йог . -®26 РМЦ 791 0.0 andbnghter 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 80 8 5 9.0 9.5 9.7 P,07-7+7.8 &V447 • • i • 4 • • » — • ♦ • • • €• 'I • • • ♦ 17^ — • •8 (MO) ♦ ® . • 20 7133 Be 93 ® EM • *| •• ’ 7160, 7139 +70° • V433 • vd8143 [j] ®V431 +68’ +67’ 7129 V434 • +64’ 22hl$m ?2h08m 21 h44m +62“ 21h36m и Nova Q Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Variable Stars S ® ® © ® ® (•) ® ® (•) ® ° Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. Individual members are plotted it separation exceeds 60" Copyright } 987-2001 Willmann-Bell, Inc.
АЛ 6* Alfirk +70° +69° +66° +64° +63° V433 vd8/43[j] +68° +67° +72° 21h36m 21h28m 21h20m 21hl2ni +74° +71° AX ®V431 . sa 6<J° ® \ +62° -----•--- —•—1 — 21h36m V430 21h28m 20MBrn-> , 20bb6ni 2^04^ 21hl 2m z 21h20m +73° CEPHEU • • • • • 5 • ♦ • • • • <• • • • +65° ® GK 7023 0 Uli 648 6 (V382) • U11678 <= OU11689 0- M+'1'25'5 0 \Ц15 .<’69^ 61° 2^^ WH Tvion / Barry Rappapurt / Will Rctnoklus
10 0.0 1 Individual membecs are plotted «ndbnghte 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 it separation exceeds 60" П Nova Q Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) | Double or Multiple Stars Variable Stars S ® ® @ ® ® (•) ® ® (•) ® ° Amplitude Amplitude Amplitude Amplitude 1.0 maq. or less 2.0 maq. 3.0 mag. 4.0 mag. Copyright 1987-2001 Willtnann-Bdl. Inc.
60 T +66’ +65° +64’ HS DRACO +62° 19h12m A2301 6650 6667 6A° 1.4763-^V' • 6676\ C341-10 0 a UU377O • • ,fzm 18h48™ ^40™ 19h12m 19h04m 18h56m r— +74° r RR ^h40m 18h48m ,61° 6651 1803*676 „НО D^C° фЗОЗ» ЗА \+11° U11334 Lun331 6654A +73’ +70’ +68’ 57 8 +67’ +69’ +72° +63’ 0 6786 • UH 402 +71’ ♦ ° 6747 ' • • • • • 1 • 1 1 52 \) . 1 U11363i * * 1 . 1, U11411 0 • • /' '<• L_ А23П • J . BF • • A231S • • • © * EE • • • ♦ • • • X ~ •» • / X / • \ • • ' / 4 ✓ Altais • • • • HQ lb ”. • • • • • «• • • • oSZ • 55 • • • • • • ’• -4- • • * • • • • ♦ • • 0 676. • ? • • • ♦ I» • • •• • • • ж -ф * • ____ 19h04m A2312 6654 -"44 X 2 • 38 • U11208 6636 U11230 6536 P94.0+2 7 • Open Star Clusters and Asterisms kJ О £' to scale < S' Globular Star Clusters ф ® ® to scale < 5’ Planetary Nebulae -ф- <> -Ф- ♦ >30” 30-10” 10”-5" <5’ Bright & Dark Nebulae ° - to scale 1O'-5‘ <S' Gi ^0 > S' to scale laxies ООО 5 -2 2 -Г < Г major axis Galaxy Cluster •ч xi to scale 17h52m to 20h32m +74° to +62° DRA CEP И/W Tirian / Barry Rappoport / Will Retnakkn
0.0 arid brighter 0.5 +73’ +72’ +69° 46go +6s° +64° Ч30 'Я18т IZI>2om i-2^h08m r"'-J8h00m /^CoT^ 6461 1622 М+12-16-12А о/е +67° GN' +65’ 20 +64’ U10731 6260 6275 +63’ 0300-14 . 6299 17^20m 17h04m 6SJ8 О О 6317 о 1.1241 о U10614 19 h * . U10736 0 ?66° • 0 • 1.1235-----< 6247 +68’ U10587 6248q +62° 'I'Ve.,--. 81 ]i/ UJ’O66 U10912 ' 6601 U10803 0 U10713 28 (и 650s О 643S 6488 686SB . 636SA° 17h28^ 16h56m 16h48m +74’ CP® । • • • • и 26 j: • • • 1 • TV 1*2255 6319' W+10-24-101 ---------о 17hl 2™ Amplitude Amplitude 1.0 mag. or less 2.0 may. 6303 6289 0’ 6288 +71’ +70’ +69’ . DRACO • ' 6244 1 +62’ 16h56m 16h48m Amplitude 3.0 mag. Amplitude 4 0 mag О A X Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Nova Quasar Radio Source X-Ray Source Individual members are plotted 1-5 2.0 2.5 3.0 3.5 4.0 4.5 5 0 5.5 6.0 6.5 7.0 7.5 H O 8.5 9.0 9.5 9.7 I if separation exceeds 60’ 1.0 CopyngM© 19Ц 7-2001 Witlmann-Bdl, Inc
DRACO +73° +72° +71° +70° +69° GK +68° +67° +66° +65° +64° +63°. 65° S949 U10383(9 U10425 0 6236 0 6232 О O6248 69° 16h48m 16h40m 16h32m +74° o • M+11 -20-28 A 6^ 3 6094 6079 C339-6 1.1228 18 g 1"^ А5'пДА6' U10561 . 16*00^ 16h08m )6hl6n' 16h24m 16h32m 16h40m 6011 О Г? i.ll47 ‘ \ I.H46 6247 c----- . M+10-24-52. ® 6^Гб238 '^10536 +t)Z 16h48m 3C343.1 U10518 1.1216 U10497 U10502 *U10503 U10162 6071 09944 U10072 6048 0 15-39 Q • 1634+706: U10476 о L/10478 LI 225 о 1.1215 uio°52- UlOOl8 0 z U98?6 1.1218 U10078 1)9992 M+11-20-16 .o ®_ ________ 3C343 • Q ol U10449 1.1214 U10294 6140 6024 6019 J M+11-20-8 1)10231 II10194 U10334 « 1)10298 6111 °i.1210 M+1V19'21 -м-!Йда 6015 . Wil htfun i Bcuty Roppaptyil / W>tl ReincikliA
12 5819 +7q° *6Оо +67° +6j° * ^78.1 +24^44п, ) / JSh04m j 1огрг : 8836 5671 М+11-18-4 DRACO FP о EK EU z-7100 15h20m ^5h04m Nh56 1.1049 I4h48m 14h40m 14h32m 1435+638 Q М+10-21-17 о 1Sh44m О U9896 Pherkad 9* K309. 1 588/ U9734 RR о FR £ochab 14h40m 14^32m 14h24m +74° 1 ~d ‘ U9529 1.1046 +73° +72° +71° +70° +69° +68° +67° © i • • .URSA MINOR +66° • • u 5807 o . U 065 +65° +64° +63° URSA MAJOR ----- +62° 14h24m Stellar Magnitudes (V) • ••ФФФ9**<**«* 0.0 dndtx^icr 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted it separation exceeds 60* Variable Stars О ® ® ® ® (•) © ® (•) ® © Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. и Nova Q Quasar Д Radio Source X X-Ray Source Copyright ft 1987-2001 Willmann-Ml, Inc
12 л URSA MINOR +73° +72° +71° +70° +69° +68° +67° +66° +65° +64°. +63° 14h00m 33h52m 1'^'5344 ° bA° ]4h24m 14Мбт 14h08m +74° i—------r--------Г" l)8374 5620 bV .19-27 DRACO 13h36rn Uh52m ]4h00m 14h08m 14h16m M+12-13-34 M+12-13-31 & 09039 5205 \ W о 08511 °5412 • • 1 • • • 1 • 1 u 5340 1)8732 О 1)8525 5607 5479 Thuban ii a .о 1,954 U8823. . U8737 5283 1)8604 5413 08894 5034 08201 +62° --- 14h24m ajrsa "1)8491 \ 5218 о о 5216 о . 08467 0828] су" o821A \ го ♦л л * SW ; Open Star Clusters and Asterisms О о О to scale < 5' Globular Star Clusters ф ® Ф to scale < 5' Planetary Nebulae >30’ 30"-10’ 10"-5" <5" Bright & Dark Nebulae □ □ □ □ to scale 10'-5' <5' Ga >5’ to scale laxies О о о 5 -2 2 -r < Г major axis Galaxy Cluster to scale 13h04m to 15"44m +74° to +62° UMI DRA, UMA WH Ttnon / Barry Rappoport / WiH Remokkib
13 +63° / 13h20^ U7767 М+12-12-7 ' +69° b +68<> +6S» I о 4120 4034 о о AS +73° +72° +71° +70° 4236 +69° +67° О +66° о RV +65° 4510 +64° 4205 o DRACO 4238 * 76л >2h4Qm 12h32m 12^24m 12h16m 0 4250 0 4391 4441 U7153 о C315-17 4108 В о U7179 о Q4108A 4108 ^IL] ^2^4gm 4512 . 11-15.54 08232 ^Q-U8234 S°07° °U82j4 ф M+f0. s0j4 '836 ^,0-'8-89 0.0 jndtxKjhtec 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5 0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 4857 U7941 о U80$2 4750 <7,4693 U7730 0 ^^848 ..'4545 '7^40^ I2h32m ~^^^ ^7h24^ 12h16m 12h08m 12h00m +74° U7908 <>07809 ’ ~a448] 'FK 5K‘g) U7490 4 • • • ®4CQ W • • • ЗС268.Ц • • ♦ • • о U7164 4128 +68° 4221 J_U7242 4210 • 42S6 Ш11-15-36 . • </25* __ ___ 4121 • • • • • • ♦ 4081 о Gt • • • 3C268 U7020A • ukamaw • — —•— +63 1.758 0 • U7019 °л 1 0 U7009 4041 о +62° 12h00m 12h08m Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. n & A X Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Nova Quasar Radio Source X-Ray Source Individual members are plotted if separation exceeds 60' Copyright © J987-200I Willmann-Bell. Inc
13 > A1412 3C268.1 A1382 \ 2 -DRACO M+12-11-42 0 C334-50 12h00m 11h52m +74° --------— U6473 3516 U6552 +71° +70° Giausar +69° +68° 3622 66° +67° 3682 +66° □6179 +64° Мч-11-14-33 О 31W Hh36m 1lh44m 11h52m s> . 4C+63.15 (J6520 O' +63° +65° +62° — 12h00m 3654 U6378 0 U6530 c 3735 1133+704 396/ 3736 ьЛ4^2 дО-6/ U6698 3879 o 0 U6711 о 06764 0 U6532 • 3C263 s-- 1 X U6381 ° 0 1)6448 • GU6429 o 3668 U6534 U6316 C314-19 m+i°-16'7_7 50 0. 69° . US?'8 05932 Open Star Clusters and Asterisms О О О to scale < S’ Globular Star Clusters фФ Ф to scale < 5‘ Planetary Nebulae -ф- <> < + >30’ 30"-10‘ IO’-5" <5" Bright & Dark Nebulae □ n D to scale 10'-5’ <$' Gi >5' to scale laxies О О O S'2’ 2'Г <Г major axis Galaxy Cluster to scale low to 13h20m +74° to +62° DRA UMA, UMI Wil Tinon / Яапу Rappapon / Wilt Remakkn
14 +62° '0^ 27 *6я° U5110 о 2957 29S7A . DL © U5336 ® EN 3077,* U5302 US442 ’ (jN 38 U5530 U5277 'O'124 m URSA MAJOR 10h00m М+12-9-58 . о b~ U5210. Ш-2959 . Q 0 Us?04 <^8 08Js о U583s US724 U572y о G/? Stellar Magnitudes (V) 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8 5 90 9.5 9.7 ^'2-’0-43 ^5576 ° US520 о US497 Double or Multiple Stars ^0^24т и- ’ 10 °8т 10h00m 09h52m 09h44" 09h36m ---—г--------- +74 U541S о 3027 О 2985 +73' 22 +72' М+12-10-13 М+10-12-19 2034 М 82 09h52m U5139 о +71 +70 24 С о U5247 2031 М 81 Bode 's Nebulae О 2976 2909 +69 +68 +67' о U5244 28 • 09h44m Variable Stars О ® ® @ ® ® (•) ® ® ® ® О Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag о J U5J11 А834 +66 +65 +64 +63 — +62 09h36m « Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted it separation exceeds 60' Amplitude 4 0 mag. Copyrighr^ 1987-2001 Willmann-Bell, Inc.
14 09h36m 09h28m +74’ +73° • U5052 DRACO • 22 +72° ллб* URSA MAJOR С332-33 2641 0 1.529 U4967c ” 2810 о 1.520 о \c332-2? 2636 1.2389 °2646* 26.30 255OA M+12-9-37 О U430S ф 24 DK d U4739 66° U5029 U5028 (J4836 О U4951 69° U4944 Vt U4376 M+11- 41V U5033 c 0?^ 23 h 0^ OFF * 5b 08b4&m M+10-14-8 08hS6m "M+10-14-19 09hl2m 09h20m 09h28m 2880 О . ... M+11-12-10 ’ 2820qc2814 1.2458 ch 2805 EZ +71° +70" DL® +69° +68’ +67° +66° +65° +64’ +63° 2892 +62’ - 09h36m 2650 0 о • 0 04896 ° M+i2-9;33‘ О n40 U4981 U & о U4775 C332-26 U4687 }C204 09 2'8B 'M+11-12-8A 04420 О Q M*1 2 7424 1O-13-14__L-- 09h04m Open Star Clusters and Asterisms О О О to scale < S’ Globular Star Clusters ф ® Ф to scale < S' Planetary Nebulae >30’ 30"-10* 10"-5" <5" Bright & Dark Nebulae <?<:? □ □ ° - to scale 10 -5' <5' Ge ^0 >5' to scale laxies OOo 5'-2' 2'-r <r major axis Galaxy Cluster О to scale 08h16m to 10h56m +74° to +62° UMA DRA, CAM Wrf Гмюг1 / Вогту ftappopoft I Will Bemokhi
U3858 (73975 (74067 «4050 1.2184° ЗС184 (73984 2366 § ЗС179 6 (73979 (74098 (73991 2403 174021 U3894 U3893 U3836 (73919 U3886 U3909 (J3859 07*36" 07*2g <>в*оо» • «4080 Т~ ‘ U3968 (74023 °. ’ М+' ’-10-37 (74094 , - U390s о (74015 I M+10-Jl М+,0-1!°цп ' ’ м+1°-п —-^130^03978^ 07^4^т U3864 Гт о ] U3838 ' ® 49 вс U4059 (74001 i • / 14+10- Г+10-12-28 °^00пГ"~'~~ М+11-9-50 <2309-35 ° j. °. Ч U3850 Double or Multiple Stars Variable Stars « Nova Stellar Magnitudes (V) andbnqhter 0.5 1 0 1.5 20 2 5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Individual members are plotted if separation exceeds 60’ В ® ® ® ® © (•) ® ® @ ® ® Amplitude Amplitude Amplitude Amplitude 1 0 mag or less 2 0 mag 3 0 mag 4 0 mag Q Quasar Д Radio Source X X-Ray Source Cupyviyhf Ф 1987 2001 Willmann-ftell. Inc
+73° +72° U3644o +71° +70° +68° +67 +66 +65° +64° +63’ CAMELOPARDALIS U3705 0 U3714 Д566 +69° 07h12m 07h04m 06h56m +74’ 1/3717 •. U3642 U3660. oES 4564 43 tw 06*2^ 06h40m 06h48m 06h56m 07h04m 62° +62’ 07h12m M+11-8-25 0?438 m+1.1'8'27 06^2" U3453 <= U3701 U3697 ~ Integral Sign Galaxy U3626 тг ' * ER I 0 U3575 0 U3580 1)3474 0 UJ403 03415 U3416 о AW ‘ U3539 U3577 c M+11-9-21 U3606 . M+10-10-21 & 03402 ♦ 0 1.445’ • 36 033*6 2253 \ Ь U3502 U3511. \ о ; Mr11'8'45 -50 \ - 03458 Q \ М+1Ц43 03478 <a tN" M+11'8' OU3437 03436 WM''-8'12 Open Star Clusters and Asterisms О 0 0 to scale < 5’ Globular Star Clusters ф ® ® to scale < 5’ Planetary Nebulae <> < < 4- >30" 3040' 10’-5" <5" Bright & Dark Nebulae □ D::: to scale 10’-5’ <5‘ Ge 2^0 >5’ to scale ilaxies 0 0 0 5-2' 2-1' <r major axis Galaxy Cluster to scale 05h52m to 08b32ra +74° to +62° CAM UMA WW Tinon / 80/ту Лпррарогт / Witt Remakkn
16 +62° °бЬ08т ® А527 U3259 +69 ° о 'О О ^3317 .^78mQ^2Qm 05hl2m 05^0401 ! . Г- BN °3h44m n . ___°5h36m U3245 67 U3235 ° U32S0 05h04m ^3349^^344 ли-.': 407-is О "3307 •W/9 AS О ^07-Ю ,D(J 05620m 05h12m 04h56m 04h48m +74’ о U3252 U3218 о I- ; • • Cr464 U3150Q • • • • О3147Г • 0 • Ш/82 • • • • • • • • • • • • • • • • • ♦ • ♦ • ♦ ♦ • (/3/89 0) • U3163 • 1.396 0 •• ^ST • ♦ • • ♦ U3 J 76 0 • • 1 ♦ ® 9a • • • • • • *• • • • • • U3167-° • • .DP • Л • • CAMEU • • • DPARDALIS • 04h56m ® ® © ® ® (•) ® © (•) ® О +73° +72° +71’ +70’ +69’ +68’ +67’ +66° +65’ +64’ +63’ +62’ 04h48m H Nova Q Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Individual members are plotted it separation exceeds 60“ Amplitude Amplitude Amplitude 1.0 mag or less 2.0 mag. 3.0 mag. Amplitude 4.0 mag. and brighter 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 80 8.5 9.0 9.5 9.7 Copyright© 1987-2001 Wittmann-Bell, Inc.
1€ о +73° U3 +72° +71’ +70 +69 +68’ +67’ 6*° 6V ,0 04h48m 04h40m +74’ 0^52^ Oi ' 04h24" 04M6* 47 © DK 1.356 1469 DG . U31I4 ©^ RY +63’ одьоо1" CAMELOPARDALIS 04h24m 04hl 6™ 04h32m 04h40m 0 U3092 62° >0 +62’ L 04h48m U31 о из 1 so 1573^ > U3069 DN 2U3143 U2865 028.00 \|W U3J63 О +66’ +65’ +64° U3149 • 1560^ • U3O9O О ? 03048 • O U3042 О .oU3046 с1569 U2916 1128^ 1485 1502 • U285V. U2826 . U27»9 ое10 Open Star Clusters and Asterisms О О ° to scale < 5’ Globular Star Clusters фф Ф to scale < 5' Planetary Nebulae >30" 30--10" 10"-5" <5" Bright & Dark Nebulae n [:• □ □ to scale 10 -5’ <5' Ga >5' to scale laxies О о <+> S -2 2 -r < Г major axis Galaxy Cluster o to scale 03h28m to 06h08m +74’ to +62° CAM CAS Wil Titian/Rarry ftappapon / Will Remaklus
. CASSIOPEIA *69“ *6<?« 8(3/о +66° *65 о +63 *6> +240^4 4 m +73° v793 +72° +71° RZ® Rx +65° BD +64° 886 +63° °^h20m c>V794 03^04^ 02h56m 02^48т 02h32m / ^SOo: / 0 " ^<?73 ^05 Cfi UsL^sIOpeia^^ 03h12m'~'-— andbnghtH 0.5 1.0 1.5 2.0 2.5 3 0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 011'12'П 0^4. 0гк56т 02h40m 02h32m 02h24m +74° SU ф QvdB8 TX V79J • • 0 • • • • • • • 0 V7£ • 18 • • • ♦ • • » • • r • • • • • • • • • ♦ • • • • P132.4+4.7 9 • • ’ +70° +69° +68° +67° +66° J. 1808 02h40m 896 1.1795 S +62° 02h24m @ © ® © © © (•) © ® (•) ® © Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag 3 0 mag 4.0 mag Stellar Magnitudes (V) Double or Multiple Stars Variable Stars n Nova N Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" Copyright © 1987-2001 Wittmann-Belt. Inc
11 ml Tirion / Barry Rappapwi I mil ЙетаМиз
18 Stellar Magnitudes (V) • 0.0 andonqhw 0.5 1.0 1.5 2.0 2.5 3 0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60’ Variable Stars • ® © @ ® © (•)(•) ® (•) ® © Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. « Nova ® Quasar A Radio Source X X-Ray Source Copynghl К) I VS 7-2001 Willmann-Belt. Inc
Open Star Clusters and Asterisms О О о to scale < S' Globular Star Clusters ф © Ф to scale < 5' Planetary Nebulae >30" 30"-10и 10"-5" <S" Bright & Dark Nebulae □ □ о - to scale 10-5’ <5‘ Galaxies о о о 5’2 2 Г <Г md|or axis 01 hQ4m t0 22h56m сдз +63° to +51° AND.CEP, LAC
19 Stellar Magnitudes (V) Double or Multiple Stars Variable Stars « Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" Amplitude Amplitude Amplitude 1 0 mag or less 2.0 maq. 3.0 mag. Amplitude 4.0 mag. 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 80 8.5 9.0 9.5 9.7 Copyright © 1987-2001 Willmann-Rpll, Inc
Open Star Clusters and Asterisms 0 Q о to scale < 5' Globular Star Clusters ©ф Ф to scale < 5' Planetary Nebulae -ф- <> <> * >30’ 30"-10’ 10’ 5" <5" Bright & Dark Nebulae □ ::: to scale 10' 5’ <5' Ga ^0 >5 to scale laxies О О о 5'2' 2'1’ <Г major axis Galaxy Cluster to scale 20h56m to 23h04m +63° to +51° CEP CYG, LAC, CAS VW hnon / Baity Huppupoit / Will йепюккл
20 20*48 20*40 20*32 20*24 20*16 М+10-28-17 ^2129 U11557 М+10-29-3 6916 С282-3 V2120 V2124 1/2112 Сус^и. &3C4J8 20*48 20*32 6939 Uli 583 draco I ’ U1L539 Amplitude Amplitude Amplitude 1.0 mag. or less 2 0 mag 3.0 mag. Stellar Magnitudes (V) Double or Multiple Stars Variable Stars n Nova S) Quasar A Radio Source X X-Ray Source individual members arc plotted if separation exceeds 60’ Amplitude 4.0 mag. 3 0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright © 1987 2001 Wittmann-Beil, Inc.
20h00m +63° I9h28m 19h36m 19h44m 19h52m +61 • 0U11502 9 • V2100 24 \|/ +60° +52“ +59° 3^56S,3° +58° 6796 +60’ +59’ +58° U11492 ,XZ +55°* +54° 6798 +53° l9h2Om 19h28m 19h36m 19h44m 19h52m +63° +56° +57° +51° 20h00m M+9-31'20 О \ VI762® 21 гМ+9-31'21 48 +62° ♦ • ♦ DRACC • • • • ) • • • • • • • • • • ► • • • • • • • 6831 о ° 6829 ... 4 CYGNUS ’m+1 0-27-12. ' 6787 о 6750 • • a 1 —— • • • • • j • I ф 1 • • • > 6856 * *6.82t о ’ __ ♦ • cu. ♦ • • • • V1579 •- ®V1351 . • • V2089 ' - ж • . •— _l ° —Ф © .^14-) \Г V548 oV2096 V697 +56 1)11435 VI817 ® V21O10 +52° J +53 ^56w Open Star Clusters and Asterisms О о О to scale < 5’ Globular Star Clusters ф Ф ® to scale < S' Planetary Nebulae <><><+♦ >30’ 30"-10" 10’-5" <SH Bright & Dark Nebulae <2?c? a a ° ° to scale IC-S' <5‘ Ge > 5 to scale laxies О О о 5'-2' 2'-r <r major axis Galaxy Cluster Io scale 18"56m to 21"04'n +63° to +51° CYG DRA, CEP И/if Tinon i Barry ftappopaa IVWJ RerrakJus
21 l?h04m 18,14Qm 18h32m 18^24m 18h76m 18h08m DRACO +60° +59° +58° 51 ° Ho 6542 +61° +60° RU. +59° . HL +58° 45 d +57° +56° +55° +54° ' M+9-29-52 +53° ^9-31./' Q +52° M+ 9-3 0-9 I Shjgm J 8640m 18632^ 18h24m 18h16m 18h08m U11241 0 . -© CX ’ Ull34~r 0 670/ RR 6687 +56° 46 c 6691 ° Uli292 I M+10-26-3 9 Uli 215 6670 T+'°-^-43 18h00m — +63° M+10-26-6 +62° +5 7° ,9h04m 6601 ,.o, 6608 V 6/92 66/7° 55'6607 66096597 °6594 • • • • ♦ ♦ • • « 0 M+10-26-17 •- • • • ♦ • • CY । A2293 ( ) • * * . > • /. 1286 C279-3 Amplitude Amplitude 1.0 mag. or less 2 0 mag 6562 -6566 6532o +51° 18h00m ° Nova Q Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Individual members are plotted il separation exceeds 60‘ Amplitude Amplitude 3.0 mag. 4.0 mag wdbr'qM" 0.5 1.0 1.5 2.0 2.5 3.0 3 5 4 0 4.5 5.0 5 5 6 0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright Л 1987-2001 Willmann-Bell. Inc
36h56*,y 18h00m +63° 17h52m +60° О . +62° +61° . * 6516 • М+10-25-126512 652/ . • 6488 _ ° 6542 6462 ° 6493 6491 1.4669 | • .6510 С • • • 6464 U11028 . ^6489 • • M+10-25-104 +57° +59° +58° • "6497 • • • • • • То U11O36 • • • Grumium • +56° +55° +54° +53° +52° о 6532 • V 0 UW С о GV 33Y Etamin i7h20m I7h28m 17h36m 6299 17h44m C300-14 26 UJ0936 010880 641 IP 6390 о 6381 GM . U10822 о 6473 ? 6449 M+9-29-23 M+9-29-14 M+9-29-42 6385 6436 0 1.1267 0 6418 о 6394 U10888 о 010770 о М+9-29-31 М+9-29-36 о U10988 6365ВЭ 6365А >435 М+Ю-25-81 +60“ +58“ +59° 6377^ 6376 010869^ *М+10-25-32 1.1258 'gfj-'V ол*сО ' 6393 6399° 6459 „ О .6454 U10971 О 6479 \N1 6386 0 >56* A7hU* 17620™ 17h28m 17h36m !7644m . 6466 о . 6478° U10984 • М+9-29-17 с М+9-29-16 О ______— +6А° 5U10796. ° 6359 M+10-24-121 С299-48 ° ’ \ 6292 Z11П 1 <?-— 6307« 6306 6295 M+i 0-24-91 6361 010830 О М+,ЙИ4 0 M+10-25jl4 6373 ^М+1,0-2-1J 6391 ° M+10-25-46 0 ил\г 6382 M+9-28-45 м+10-24-123 * О U10811 Draco Dwar*o 6338 6345 » 6346 24 V’ Rastaban М+9-28-43 О U10821 U10839 GQ . 3C356 010687 Gio648 м>-24-8 М+Ю-24-87 U10646 U10758 M+9-28'31. ,,,8 М+9-28'30 63зо • . о . 6286 м.р4*- : м^-28; ь 010644 K\TaW +51° 18h00m 17h52m Open Star Clusters and Asterisms to scale < 5’ Globular Star Clusters ф© Ф to scale < 5' Planetary Nebulae >30’ 30’1 O’ 10’-5" <5" Bright & Dark Nebulae <2?<P □ □ " “ to scale 1 O' - 5' < 5' Gc >5 to scale laxies ООО 5-2 2-1 <Г major axis Galaxy Cluster to scale 16h56m to 19h04m +63° to +51° DRA HER
22 l2h04m 16^32m 6247T" l6h40n • 6258 о Ww 58 6223 . О / U10517 •^'0-24.9j . 3^3 e 3C343 1 ° л. 0 U10449 1210561 6238 о U10536 .° 6226 ] • u>0542 +60° °rx 16h16m 16h08m 16h24m M+10-23-75 1 1 • • _ / • • 0 1.1210 • • 1 0 г 6123 1 ° C298-22 О U10284 °° 6095 16h00r — +< DRACO +6 +6 0'0590 +59° ^6189 “6176 М+Ю-24 6286 ® oCl M+10-23-68 13 0 6190 M+10-23-72 6187 6127 6198 M+10-2 3-23 * U10408 .° M+9-27-4 Irakis 21H M+9-26-53 • • +51° U10271 0 о U10548 О M+9-27-27 M+10-23-85- __о 6182 . M+9-27-47 AT U10331 . о 6088A 60888° • M+10-23-54 c ^M+9-26-52 °U10214 U,0646 0 +928-]9 U10510 +~10-24-32~r 6713 4 , ♦ U10279 0 M+10-23-53 c M+10-23-\ c. 6130 U10361 6136 I ъ M+9-27-31 ' <биЮб87 0648 421! 6206 +6 +J — +: +5 +5 +5 +5 И2 +5 1.1211 6090 +5 U10129 c 1/10396 U105 //° /6^4 gm 16^32m 16h16m о EV M^9'27-69 M+9-27-68 M+9-27-58 . • — — 1 0 M+10-2. ° u •39 ’ 0247 ф 6246 6246A . U10644 *GL • ^10601 ?00+si8 DrACo ° / 1110515 . U10454 M+9-27-50 [6143o. • • • • • • • • о М+9-27-13 о • • M+9-27-18 —^.•_M+±27-[2\ , M+927-26 16h24m 16h08m —1 +5 16h00m Stellar Magnitudes (V) 00 and better 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60" Variable Stars О ®> ® @ @ ® (•) ® © (S) ® 0 Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag 3.0 mag. 4.0 mag « Nova Q Quasar A Radio Source X X-Ray Source Copyright^) 1987 2001 Wittmann-Belt. inc.
16h00m +63° i5h20rn A 5h28m 15h36m BV +62° +61° +60° Edasich 121 ’ • +59° 13 6 +58° +55° +54 +52° 1 +5»° Ж +57° о U9J33 +56° +53° " 11100 5894 1.1099 M+9-25-29 3C319 о U9663 M+9-25-31 3 5875A- • U9722 д 5^04^ DRACO I5h28m 15h36m 15h44m 15h52m +51° L-HERCULES 16h00m +56° +59° +63° М+10-22-Ю (/ 5907 bOO^tS J a-SA f U10129 4 U9°629 \ J +52° 15h52m • 15h44m DRACO • • c • 3C325 A e 60/5 . • 1 •J ♦ U10031 0 oFY • • • • • •1 • -— — —— - 1 • • • ♦ • • 3C323 * 1 . A 1 © • • • ___ —'# “ — — e о M+10-23-9 • • 0 M+10-22-38 M+10-22-22 , ' »” S,81 ' o0 “5976 5,85 S9!2 . • ————- • • • • 5987 FX • 1 — - • • "" • • ♦ • • • • • • FV * • • m+1 0-22-21 О • • • • • • • • 59 5965 % 5963 71|<7O 5969 ° • • • • • • M+9-26-18 0 • c • 0 U10013 • — • !3C322 A * M+9-26-32 • • • • • • • • ' • \ !• • • 1 • M+9-26-27 M+9-26-24 ’ M+10-22-9 1)9638 .Bu 5879 5905^ о M+9-25;37 5908 о ’ \ ^759 ,5866', о 5862 0 5870 ' O U9737 5874 5876 М*9-25-П M*9-2S-15 о M+9-26-12 о BOOTES U9849 U9853 M+9-25^h 5875 О M+9-25-36 О АП ’ М+9-25-22 U9702_ Open Star Clusters and Asterisms О О о to scale < S' Globular Star Clusters ф ® ® to scale < 5' Planetary Nebulae -ф- -ф- -ф- < >S0" 30*-10" Ю'-Ь" <5* Bright & Dark Nebulae <?<'?/ □°::: to scale 10'-S' <5' Gc A >5 to scale laxies О о о S'-2' 2' Г <Г major axis Galaxy Cluster »ч A to scale 14h56" to 17h04m +63° to +51° DRA BOO, HER VW Tirion / Barry Rappoport i 1ЛМ /tanoWus
23 ]4h56m l4h4Qm I4h3?m 14^24m 14,h16m 14h08m 14h00' M+1 0-21.,17 DRACO +60° +59° +58° +( +1 +. FO ' +! U9688 Кзоз 30295. M+9-24-3S 23 e '4'5бт 17ku I4h48m BOOTES URSA MAJOR I4^24m 0 5475 U9071 5422 О 0 5624 U9060 5443 о U9032 5486 * ^ 5484 . о M+10-20-78 •....fJ - - - - Ch M+9-23-47 °4 M+10-20-5 ------- + / ^-5207 I - M+9°-24.+29624-22 ^448 o. l4^4()m ""•------—. ^1999 / 1069 - 5485 0.5473 0272-32 S457M101 • 6283 DfMCo 60 BU U9663 U9629 «>D( W988 U9SS6 о U$>638 ° 5229 0 M+9-24-34 5682 M+9-14-54 *5281 m+10-21-/q о (79391 U9412 0 5667 »; • • • • ♦ о 5503 5540 • • • • •— • • ♦ • ♦ • — J8985 о о 5561 • • • • • IU о M+10-20- о 79 • f • /WJ '"60 5526 о М+10-20-84 U8970 a5631 q5585 . M+9-24-/7 о o M+9-24-22 1-1027 . &M+9-24-ii M+9-24-/2 14^32^ о (79245 Q 1418+546 M+9-23-61 (79178 14h16m M+9-23-51 n М+9-23-52 о о M+9-23-42 14h08m Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 5477o 5471 5462 : 5461 —+—5458 5455 5451 5451 о M+9-2 5449 5447 . 5450 5474 14h00n в Nova •) © О О Quasar Amplitude A Radio Source 4.0 mag. X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Individual members are plotted if separation exceeds 60” 0.0 and brighter 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7 0 7.5 8 0 8.5 9.0 9.5 9.7 Copyright 198 7 2001 Willmonn-веИ, Inc
2 14h00m +63° -|3h20m 13h44m 13h52m о RR +62° +61° +59° +58° +57° +56° 51В °о 5109 +60° +62° +58" +89° +61° 13h28m ---------- U8491 U8467 5205 о U85H M+10-20-19 M+10-20-23 . 5370 29 M+10-20-16 78 M+10-19-86 1.942 4977 5164 ' U8671 41783' IS ® 83 IQ IR 84 CR 1/8658 Q 4C+58.29 5342 о U8741 -vs- 5308 —Q>-- U8892 5368 о U8882 о 5294 о • М+10-20-36 о • 5372 U8886 О о М+10-20-11 (3i4Ci55.27_— М+9-22-79 ' U8508 О М+9-22-74 * М+10-20-21 ° • U8714 о 5322 . • М+Ю-19-94 I о ° • М+9-22-84 о М+9-23-9 22'^79; 80 0 Miza' CQ® 5255 М+9-23-3 . • ___. • 52795278 +60° 5402 0 5422 О +55° - •0^5379 5389 oU8859 5430 ° 05376 0 М+10-20-59 i M+9-23-23 5 N\+y . e 0 5001 М+9-22-1Ц^— 'M+9-22-67 0 a 4964 13h36rn _ FT52l8 Keenan's Systerri о -.5216 0 +54° +53° +52° +51° --- 14h00m DRACO U8335 U82aU8234 OU8214 О о 178837 е 86 52164 U8649 U8684 о •M+10-19-77 U8226 U8282 1.852 О 1 М+Ю-19-85 a 3C2”',CM.W-I9-I«2o. 41767 О M+10-19'71 U8205 M+10-19'14 82 EH® M+9-22-92 URSA MAJOR 13h44m | 1.952 13h52m oo 5204 М-И0-19-?5 U8441 М+10-19-7? o U8551 520Ю CANBS VtNATICI .5238 „ 5225 M+9-22-65 о I.875 1)8058 13h36m U8339 M+10-19-49 ^’n’00 U8231 о 21-94 1)8107 о .А \°М+9' 4967-^+9-22-3 © О I 5163 М+9ША"'-л М+9-22-54 М+_9^22-44 , ’ М-+9-22-36 1.853 U8^1 oCK ^04rn -|3h20m M;9-22-41 M+9-22-35 О * M+9-7Z- М+9-22-23Г U8211 4834 13h28m 5040 о 4938 Open Star Clusters and Asterisms 7"'"i Г) C) to scale < 5' Globular Star Clusters ф ® ® to scale < 5' Planetary Nebulae -0- >30' 30"-10' lO’-S" <5" Bright & Dark Nebulae □ □ □ :: to scale IO1-S' <5‘ бг A >5' to scale laxies О о о y.2' 2'-Г < Г major axis Galaxy Cluster 'v 'j to scale 12h56m to 15h04m +63° to +51° UMA DRA, BOO, CVN И/i/ Гггкх» / Burry Hufjfx>por( / Will Remuklui
24 ^h56m 12h48n l2fl4Qm I2h32m 12h24m 12h16m 12h08m +60* 458° +56° yh04m 76 • ‘ 4605 <2292-85 4036 ®RV • ° 07064A M+10-17-147 ,.p 4199 ° 4195 ’ A1496 4814 • 7S o/M 07070 о 07659 78 (77922 45/1 73 M+9-20-96 о M+9-20-130 ' 84 • 4384 70 4566 1-830 . M+9-20-138 4732 ° M+9-20-91 <>4181 oM+9-20-131 M+9-20-151 I 68 M+9-20-153 4707 '^h56m I2h4gm 12h40n О 4194 '(J- U7218 4142 0 4172 o 4161 <S’“ 1.801 4271 70 9-M+l 0-18-27 M+10-18-28 I U7379 • о U7144 О (71+9-20-181 0 M+9-20-1 83 о M+9-21-] M+9-20-172 ° I • 5 f. M^20-97 4102 Q 4068 M+9-20-103 WZ 1.758 0 • М+9-20-68 c> 0 / М+9-20-80 А1436' 69 S Э-_____>68 Megrez M+10-17-141 -40954 M+10-18-21 __/ ^A1507 , \A1452 07082 4-z (Ъ\А1468 M+9-21-9 О I 0 • (71+9-21-8 ' О 4141 M+10-18-6 4149 TZ 71 o 4500 07618 ^'8-89 M+1 J -15-54 0 07406 07153 ^J46 M+10-19 (71+9-2) ° U8/S, ° 4938 ^1-83 —° 4801 (7805o' ' 1780/2 M^°j8-87 . U8046 (78040 -3^.1O 4547^4549 07691 о 07635 Alioth 07993... (77950 M+9^2h32 0 4686 ^4695 4675 464 6 12h00r +< o 07019 0 07009 4041 о < +6 +( 74 о 4335 U7534 43624358 M40* гЬ4284 (rl+9-20-176 О 12h32m .0 М+9-20-157 ' M+ 9-20-155 • •-1- 12h24m M+9-20-156 • о 4198 М+9-20-108 CANES VENATICI . 07267 12hl6m +: +5 +! +; URSA MAJOR М+9-20-77 12h08m 12h00n Variable Stars • ® ® (•) ® ® (•) ® О Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 maq. 3.0 mag. 4.0 maq. D Nova Q Quasar A Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Individual members are plotted if separation exceeds 60" 0.0 andbngMer 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9 0 9.5 9.7 Copyrights 1982-2001 Willrnunn-Bell, 1гк
12h00m +63° +62° +61° +60’ +59° 11h52m 11h44m 1lh36m Hh28m д065^бУ s . 4C+63.I5 о • M+10-17-120 e U6520 о* ’ . M+11-14-33 3762 о 3471 а. • о m+io^i,6’90 +62° 0 U6080 ; +6А° 0 U6192 M+10-17-57 • U6858 0 3945 О 3975 3978 о 3543 3725 иб528 M+10-17-64 0 о 06727 о М+ЗО-1б-52 : 3740 3470 о U6762 О M+10°1 7-79 3796 <9 ,-.3835 # Л3589 \ +60° . M+10-17-97 3894о м+10-17-75 3894 . • —о U6732 о 3809 3770 о 06682 U6452 I о 3642 U6335 1.691 О M+10-16'71 О I О 361 о о М+10-16-110 \U6H° \ гг \ +59’ 3963 М+10-17-121 ‘ ^3958 О +58° +57’ +56’ +55’ +54’ +53’ +52’ 06912 U6931 ° ®Z U69S7 °“U6939 A1436 • 66 U6816 о о 3795 U6616 c U65/5 "*^3838'* M+10- 7-58 *37958 3757 106566 оу* . 3690 ® . 1-б94\ М+Ю-17-7 M+10-J6-118 L_——\ °зб1 з М+10-17-4 3625OU V ° 3669 3619 М+10-Ш4 U6767 ,„„.06919 М+9-19-196; 3998^ " М+9-о20'27 ' 3977 ^3972 ^ 3982 • U6894 о М+9-20-49 о Phad 64 уф .U6o6L 3992M109 0 U6923 о U6983 +51° 12h00m О М+10-17-19 о М+Ю-17-10 368ЗА; М+10-16-1^4 • _ ° 3674 aJ ~~~ ’ 1^3683 HQ® • м+10-16’92 ! 0-16-61 \ °M+1O-^9 +5%° -м"^4 \ <2 \ О 3488 • 3530 M+1 °;16'81 M+1O-16;122 m+1 0-16’89 L . • . \ U6228 о 3517 A,,3t^;iaus"' ®48 ?> \ 0 \ 3499__- +56° • м+9-18-59 A1291 о3780 ...9 М+9-19-’76 o3g04 3898о 3889. g_________________________1 ff?846 ° \ * HR 41377 Ursa Major! Cluster • 1 o3913 • • • 3759A 1A1318 м+9-19-126 38,6 да' —то— 06774 / ?\.А1383 М+9-19-172 0 • U6828 U6766 3953 0 U6840 Q 3931 URSA MAJOR - 4026 С268-6 R3556 Ml08 М+9-19-3 0 o0U6802 3917 G 11h52m ДА M+9-18-70 U6I860, о 3824 Г3829 3594 0 M+9-19-18' 3587.M97 * M+9-19'72 M+9-19-752* ''/1218 'о U6309 НМ ® 3631О 3657 0 3729 О фЗЛ8 U6527 U6505 i О О М+9-19-97 М+9-19-49 о М+9-19-44 А1270_;_ -Г^--'\М+9- U6518 U6446° ^373зТ-,9^12\ ° М+9-19-125 ^3738 • 3756 о M+9-19-16/J U6667 U6555 11644m 11h36m , М+9-19-42 0 V М+9-19-'6 М+9-18-102 M+9-19-73 ;T3656Z..A1225 ”'64-’ ua5, М+9-19-52 Uh28m М+9-19-5/ М+9-Г9-5 Arp's Gotoy М+9-19-68, — -J--'"' ддЬ20т о 3549 u6182 q 18-84 о M+9'’*? M+9-18-’5 M+9-18-72 \ +53 Open Star Clusters and Asterisms OO 0 to scale < 5' Globular Star Clusters фф Ф to scale < 5' Planetary Nebulae (><+<> + >30" 30"-10" W-5" <5" Bright & Dark Nebulae ° to scale 10'-S' <5' Gd ^0 >5' lo scale laxies ООО 5-2' 2'-Г <Г major axis Galaxy Cluster \ 'j to scale 10h56m to 13h04m +63° to +51° UMA CVN Wd 1 it юг> / Buriy RupfXipoa / Will Remakkis
25 ]0^5бт +5]° 1lh04m . 10h4Qm 10^24т +6/0 +60° M+10-15-51 3102 и • 0 co +58° M+10-15-34 M+J 0-15-90 +52° 3225 0 , U5534 о 3182 \lh04+n +62° Dubhe 0 U5435 U5542 oJJ1 3168 • 10h08m Cr C312-32 М+10-13.93 ' GR О‘о U5475 US480 ->/<72 3470 •GU Ю 5408 5488 '49 40 о 3164 0 C266-31 .51/ 0 US421 U5720 M+9-17-19 3310 U5460 ]0h56m ^0^4Qm Ю^32т URSA MAJOR l0"24m 3286 о 3288 0 M+9-17-33 c> U5479 M+’ 0-1.$.1O8M+1°''54 °3 0958+551 S ъМ+9-17-16 _ M+9J7-56- М+9-17-55 М+9-17-49 M+!°U5-106& . М+'0-15.104 us,24 ишз 3398 3458 14 3448 - •41 39 CV ^+92j8-24 5410 ^0^4gm 0 wo 50q U608Q DM ° US846 10h16m 10h00m — +63° U611g ^'0-16ч/ Werak OrsoL 48] ^9-'8-63; ^9-’8-70 U6016 US928 3406 м+/о.1б.;8 M+,0-l6-25 ^3440 43 о 1-646 ° M+J0-l6.9 .ex 116. ^U5848 US888 М+9-18-1б M+9-~18-14 • ivy • •[ +62° • • • ———J 3236 • • • Л 3C244.J М+10-15.ТПн м+10-15.99 п I -° о М+Ю-13.Ц8 №10'15-9б к. ,л ’ US626 М+Ю-15-79 о/ 3238 о0 I 32203-^^.- М+10-15-70 M+9-17-64 +61° +60° о о М+10-15-3 O.US408 +59° +58° M+9-18-4 US734 о . U5733 G266-48 о U5676 C266 46 ° о M+9-17-65 3188 . *3188A U5422 0 3206 М+10-15-67- M+9-17-42 o’ U5546' о U5549 10h16m +57° 0957+561 A,В Q ‘ 3079 f) ° M +56° +9-175 O 3073 +55° U5369 +54° M+9-17-11 о C266-9 U5459 ° M+9-17-26 M+9-17-23 +53° +52° 10h08m --- +51° 1ohoom Amplitude Amplitude 1.0 mag. or less 2.0 mag. Amplitude Amplitude 3.0 mag. 4.0 mag. Stellar Magnitudes (V) Double or Multiple Stars Variable Stars « Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60‘ ’ о.о andbogbtrf 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright © 1987-2001 Willmann-Bell, Inc.
09h20m 10h00m +63° i 09*32* 09h36m 09h44m 09h52m +62° +61° о 3043 291) +53г M+10- +58° M+1 о M+10-14-47 +60° +52° +60° +55° +56° +54° +59° 0^5бГбУ rw U5201 ’ ,401,ля •> M+9-16-42 M+9-16-48 , М+9-16-44 м+9-16-43 e +59° C266- 0<^04* URSA MAJOR 09h28m 09h36m 09h44m 09h52m 2739 • 2740 U4717 о • C264-90 . О, о С264-86 1)4906 ° oU4879 ’м+9-15.-1-60- . * \ .0 • 2800 2693 2694 2870 OU4932____—" o9hA2(’' 09b20m 09h28m 23 h О fF ‘ 2880 M+10-14-19 ' О U5077 M+10-14-39 ttU5179- 0 2950 CK U5013 U4973 М+Ю-14-12 M+10-13'6-6 ° 0<^04* ««SK»*'''0' 1)4730 2726 . U4788 WJ +63° ф M^lO'13’47 1)4683ji 0-14-56 +57° U5241 . U5207 YY 2895 U5106 о C265-23 M+9-16-14 • U4807 °.\Y ' 18 e о 2710 2701 О 114696 U4713 л’ U46^ х4б”г1й«Д ♦«' +51° — 10h00m 26 Г ' U5 076 М+9-16-29 •25tl .«uso« . М+9-16-30 i 2841 1)4749 o 1)4824 +53 Open Star Clusters and Asterisms to scale < 5 Globular Star Clusters ©ф Ф to scale < 5’ Planetary Nebulae । -ф- <> < + >30’ 30" 10’ 10’ 5" <5" Bright & Dark Nebulae A . ,s. <2?c j п n °::: to scale 10' -5' <5' Ga ^0 >5' to scale laxies ООО 5-2' 2-Г <!' major axis Galaxy Cluster to scale 08h56m to 11 h04m +63° to +51° UMA Wrf r«wi / Яппу / Will Remakltn
26 +6°3?h0^ 08h56m 08h4gm Ов^от 08h32m 08h24m LIS +62’ +60’ +58° Ъ'О-'З-З; U4525 m +51° °^04m . 53 U4128 ® URSA MAIOR 29 +58’ 54* +56= U4133 M+9-14-50 +56’ 0 04427 +55’ M+9-l4.6] o 0 0 +54’ • FS +53’ . CV U4546 +52’ U4499 08h48m 27 08^4Qm 08h32m 08h24™ 08h16m Ъ2701 U<696 О U4442 M+10-12-85 ----<2—___ /5 e M+10-12-130 (34277 CS> о M+9-14-17 2534 ♦ CQ . U4230. • U4293 U4196„ * 0 U4169 U4182 g 0 M+10-12-72 M+9-14-38 0 2518 LYNX — +57’ > C287-31 M+9-14-31 • о 134^357 • • 2694 5.9 M+10-12-67 +61° 268] FT, 0 °846+5]2 ^M+W-12300^ 10-12-81 •; 2 A6^ M+ (0-12-У9 U4270 752521 • m+10-12-78 134241 • 0 U4438 • U4322 j • • 1 08h08m л08h00m ж +63° I ’ 04186 CAMELOPARDA +60° u^30 W5/2 Fty 1656 2654 0 U4564 4163-70 °4690 ’ , I M+9. 0 m+9-15.21 M+lO-134 0 • • 124549 ®K205 (34478 (34514^M+9'] 4-80 FM ♦ 1 О Muscida M+10-12-94 M+10-12-109 M+10-12-8 7 FK '12-141 U4289 M+10-12-108[\ U4314O P, T*281 _M+1032-107/^ 2549 134280A^ 30 • О.л- м+10-12-120 1 • J • C0? • 2497 &Л- M+10-12-63 0 U4164o ’ 2488 L 0 (34267 . I (34280 5 • • 1 M+9-14-29 134335 . • • • ♦ • • • °8h56m , 1602 : 1603 о» ; * '2600 44515 134461 08h08m 0 2505 — +51’ 08h00m +$2 Stellar Magnitudes (V) 0.0 andbnghiK 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7 0 7.5 8 0 8 5 9.0 9.5 9 7 Double or Multiple Stars Individual membets are plotted if separation exceeds 60" Variable Stars • ® ® @ ® ® (ft)®® ® ® 0 Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag 3.0 mag. 4 0 mag. » Nova Q Quasar A Radio Source X X-Ray Source Copyright © 1987-2001 Willmann-Bell. Inc.
07^ 07h20m 08h00m +63’ +62° +61° • 53 +60’ +59’ 07h52m 07h44m 07h28rn М+10-11°-41 U4059& М+10-12-28 ©49 BC 07^36^ О o' U4001 о e>U4015 о U4024 о М+10-11-150 •М+10-11.-96 М+10-11-92 1U3978 FG О C-J3704 0 03685 "39?5 * >.03886 • U3826 BY 1)359» й\ 17 \ +63° \ ^4 M+W-l 1-126 M+10-11’70 24 7456 U4065 0 U4033 2460 1.2209 о U4013 0 М+10-11-146 2468 М+10-12-10 М+10-12-14 ° 2446 1 +60° С262-54 ’ов! М+9-13-74 b *23_ _ U3 981 • U4020 U4003 О М+10-11'53 °и389 и3885' U3928 о • U39l3 ° М+Ю-11-94 М+Ю-11-133 . М+10-11-135 J b^OzLld^^r — ____ О’ . । 24 58 U4049 о • М+9-13-67 . 2469 м+1°-12'16 _0______а________ U4121 о М+10-12-12 oBS Bl- . M+9-13-50 2431 x A595 U3792 U4071 07h20m 07h28m 07h36m U4079 o 2457 - 0 М+9-13-47 М+9-13-56 U3963 Ci U4074 CL./ М+9-13-88 Р164.8+31.1 -6- U4085 т Ci 07604,с 0 04122 Q .М+10-12-26 О • М+10-12-36 U4092 +58’ +57°------ о 2463^ М+10-12-50 2472 ° V +56° +55’ +54° +53’ +52’ U3855 • i М+Ю-11-82 ‘ М+10-114’8 U3867 ° M+9-13-17 18 м+ю-1’-42 о —— — ♦ 47 Vbxn из789 М+10-11'9 \ „М+10-11’29 U3816<3M+10’1 — M+10-11;37 U3765 M+1 O’11 \ +56' М+9-13-71 СН U4035 0 U4043 2475 ^2474 ° 04072 . LYNX • +51’ — 08h00m 07h52m C261-65 U3957 из923 C262-21 0 H3948 0 U3882 • • U3875 o U3832 • ° M+9-13'1 Ym*9-12-23 о М+9-13-63 . I2429А 2429В Ьо . 2426 07h44m BX о M+9-12-49 BU OX о U3684 . о U3627 \ ^6* о R О Open Star Clusters and Asterisms f) o o to scale < 5' Globular Star Clusters ф ф Ф to scale < 5' Planetary Nebulae -ф- -Ф- <+ ♦ >30" 30"-10" 1O’-5’ <5" Bright & Dark Nebulae □ a D ;:i to scale 10’-5' <5’ Ga <^0 >5' to scale laxies ООО 5-2' 2-Г <!' major axis Galaxy Cluster to scale 06h56m to 09h04m +63° to +51° LYN UMA, CAM Wi< Trnon / Barry Rappapan / Wdl Remakkis.
" ^’°-’0-2l °6h56m 0б^4пт 06^48rn 0б^32т 06h24m 06h!6m 06h08m +62° U3S4S *б/° U3598^ +60° +59° +58° +57° 4/+р. +55° -Z BR . -o*. 38 ® 2128 —® CAMELOPARDALIS AURIGA ° V453 °6h56m 06h48m 0б”40гп 06h32m 06h24m U3432 ° 03394 5] ° ^u3627 0^04^"—^ зз5 ° M+9-10-5 03484 03504 M+10-10-3 “ 8$ 4/+р (J3S74 (23S690* U339S М+9-12-4 M+9.J2.] <260-37 0 LYNX V382 03480 03488 0 AURIGA oV460 ' © V455 V457 • • • ♦ • 1 •“ • • • • i • * U3411 1 -й— • • в • • "f* • • warn U3382 . V ' 3> * I 1UW^ • • — *» .' • • • • M+10-9-14 • • • • • • 1 • • • • 1 ®39 40 M+10-9-6 о • • • 1.2166 о ° 2208 0m +63° +62° +61° +60° о U344S 03446 ~<&- 2UZ M+10-9-18 •5 • Р158.9+17.8 ° М+9-11-2 +59° +58° +57° +56° +55° +54° M+9-10-4 О • +53° +52° 06h16m C259-8 06h08m J +51° 06h00m Variable Stars ® © (•)<•)© ®®o Amplitude Amplitude Amplitude Amplitude 1.0 mag or less 2.0 mag. 3.0 mag. 4.0 mag. п Nova Q Quasar Д Radio Source X X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Individual members are plotted if separation exceeds 60’ andbnyhtet 0.S 1.0 1.5 2.0 2.5 3 0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright D 1987-2001 Willmann-Bell, Inc
06h00m +63° — 05*12m 05*20™ 05*36™ 05*44™ 05*52™ CAMELOPARDALIS 3 U3382 +62° +61° +60 +59° +57 +58° +57° +56° +60° +5A° +59° •21 • 23 U3 351 • 18 01 ® C+- +55’ V437 +54° «V V441 +53’ О U3375 05^ U3346 AURIGA 05*28™ 05*36™ 05*44™ 05*52m +51° "— 06h00m +52’ .„«-I ”nW 14 • C283-4 OU3218 • • • • • ♦ • • • • • • • ’ ® 31 TU Ф • • • • ^30 • • • < • >28 .29 U3354fi ®26 2013 0л • 24 +6V Open Star Clusters and Asterisms Globular Star Clusters to scale < 5' to scale < S' • • • 20 22 • U3314 С258-Ю C258-9 Planetary Nebulae >30" 30" 10" 10 "-5" <5" Bright to scale & Dark Nebulae 10’ - 5' 150V® 16 • R o* U3273 * Galaxies ЦВМ 11 ” U3260 Galaxy Cluster • 8 1708 1790 □ to scale S'-Z Z Г < major axis to scale 04h56m to 07h04,n +63° to +51° CAM AUR, LYN Wi7 Tirinn / Barry Rappoport / ИМ Remoklui
28 @ ® ® © ® ® ® ® ® © Amplitude Amplitude Amplitude Amplitude 1.0 maq. or less 2.0 mag. 3.0 mag. 4 0 mag Stellar Magnitudes (V) Double or Multiple Stars Variable Stars « Nova О Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" art brighter 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copynghf © 1987-2001 Willmonn-Bell. Inc
VW fmon ! Barry Rappoport / Witt Remakkn
29 Stellar Magnitudes (V) Double or Multiple Stars Variable Stars 0.0 txijhte» 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9 5 9 7 Individual members are plotted it separation exceeds 60" • ® ® © ® ® (•) ® ® ® © ° Amplitude Amplitude Amplitude Amplitude 1 0 mag or less 2.0 mag. 3.0 mag. 4.0 mag. я Nova Q Quasar Л Radio Source X X-Ray Source Copyright © 1987 2001 Wittmann Boll, Inc.
02h00m +63’ --- 0^04^ 0A"A2m „ 0Ah20m 01h28™ OlW 01h44m 01h52m 126” * CASSIOPEIA Be 5 Г?28 129' +62’ /.166 ..AZ Cz5 +61 26 +55° +54° +53’ +52 +58° +52° 654 •. .V771 J772£_ «/ ',m IM C/4 xz wx- 74 i 0AhA2m 650-51 M 76 oih36m 01h44m 01h52m Ж J +5V OO^ +51’ 02h00m PERSEUS CASSIOPEIA _ 0^20m ' o1h28m 271 . V539 Go^S’“'°r 366 358 Be 7 bp: 663 . +60i +59’ +58° +57° • V778 X * . о о ® . * •’ "v777 • • 1 * • 1 * • • CASSIOPEIA - ♦ • • • • • Xs) ' * • • • • • • • • • • • • 5t£ ♦ V773-® RW"”^ • • • • • _ • • V548- • Pl 31.4-5.4^ • • • • ♦ • • • • _ • , .V595 • > L„—.- +56“ • • ♦ • • Г . 39X ’ 744 • __1 (V436) V538O. X/761 ‘ X/767 381 OX 1.59 +6' XX M 103 V768 • Sh2-188 . • 1.63 Rucbbab 436 V466„. ‘ 457 № • 34 ФГ V465 X/764 \J76O” 28 J365 ♦ Ml = AA c X/555 CASSIOPEIA • • • • • • •— — — • IZ oM759 • 1 ♦ 4 • • • °TT • • • • • * i e 1 • .-Ф-Р133.1-8.6 ’• • • • • • • ♦ • ♦ • • • ♦ I* • Little Dumbbell Open Star Clusters and Asterisms О О о to scale < 5’ Globular Star Clusters ф ® Ф to scale < S' Planetary Nebulae (> <><> + >30" 30"10' 10’-5" <5" Bright & Dark Nebulae <2?o? ° °; : to scale 10'-S' <5‘ Ga >5 to scale laxies о О о S' 2' 2 1 < г mapr axis Galaxy Cluster О to scale 00h56m to 03h04,n +63° to +51° CAS PER, AND Wil Tirion/ Rarty Roppapnet / Will Remaklui
30 W52m 00*48т nnh "’----- 00 44m 00h40m 00h^m 00^32т 00h28m 00h24m +51’ +50° +49° +44° +42° +41° 0 RV >SS 0 ти .ST 0175 +49’ 278 +48’ M+8-1-251U6I 0 012888 V342 vx 0263 □ V345 0236 +43’ 0522 23 t/64 ANDROMEDA 00^48m 00^l44rn CN 00h32m SV о 00h28m 0306 °o 0303 +46’ ^M+8-1-23 +50’ 00h4°” 00^36- 0460 00h20m 00h16m 00h12m 00h08m 00h04m 00h00m —-----------------------------------.-T--------+52’ +47° +45°> +43° EC® л : JC22 ' ° U475 V/° 0486 M+8-2-12' • • ♦ • 0256 A63 0471 22 0 ®20n 0372° 0394 M 110 V752 185 0 147 9747. M+8-2-2 ' J 221M 32 . 206 (star cloud) \A72 -°BZ 0 0336 +40° 00^52m 224 M 31 Andromeda Galaxy AO ® Pearce's Star • • • 1-1-41 0 0196 U171 0178 * ° U183 M+8-1-29 •51 49 ; J/<xl048 ^31534 ’ ’V349 085 j • Ф 1 1 » ♦ 0243 • • • • V353 V352 0 . • • • • • 0Qh24m -----~ -X CASSIOPEIA , ' V348 26 0158 c 0112 00h20m 00h16m 00h12m M+8-1-27 • • • • • • • oU48 • • M+8-1-20 .0128890 M+8±ld +47 CC © 00h08m 00h04m LQ ® +45’ +44’ +42’ • +41’ +40’ 00h00m Stellar Magnitudes (V) • •••••••••** 0.5 1.0 1.5 2.0 2 5 3 0 5 5 4.0 + 5 5.0 5.5 6 0 6 5 7 0 7.5 80 8.5 9 0 9 5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60’ Variable Stars • ® ® ® ® (•) ® ® ® ® о Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. и Nova Q Quasar A Radio Source X X-Ray Source Copyright® 1987-2001 Wiltmann-8ell, Inc
23*0»% ANDROMEDA +50° +49’ KS° ' ® PV +46’ +45’ +44’ +43’ CG © LQ ® М+8-1-5 00h00m 23h56m 23h52m 23h48m 23h44m . 23^40^ +52’ 0 V394 U12809 о . M+8-1-6 c* о M+8- Bl ©ET U12517 д 3C470 BG 7618 KR +42’ V399 U12632 7640 +41’ U12634 О lO + 50° +40’ oV400 V392 •o .M+7-48-14 ь.» l’1'20"' гУ"6'’ 23h36m 2^2^22*28 ^ 2 CASSIOPEIA V814 _J +40° 23hQ8rn , _____ эзМ2т z -- — ?чМ6гп 25 23*20™ 2i - ,m 23*32™ 23*28™ 25h24m 00h00m 23h56m 23h52m 23h48m 23h44m 23 40 \j382 . V383 U123960 ’ 10 o4 ®9A? +51° • ©R • • • ♦ • • ♦ • ♦ • • • • • • • • о • • • ♦ • .. c U12851 • • • • • • О • RS . • *» • • - +48’ M+8-1-15 U12862 • M+8-1-13oQ '^U12889- +47o M+8±19_ *P 0 1.1525 U12888 .• Pl 12.9-10.2 V815 ♦ • • • • • • • 18 • V • • ♦ 1 • • • • • __ • “ЧГ U12750 1 . 1 • • I C548-1 « • • • • • • • • • ••• • i EV • • • 1 : w • •i* U12433 о 7 . % U12411 +48’ PI 0.6-12.9 U12796 TZ • © ° V396 -4 U12795 o' M+8-43-8 20 \|/ # oV395 WY BY GG 16 A, U12742 19K о I ’ M+7-48-16 171 U12669 о • 7707 M+7-48-6 ® 13 0/388) • +p-7662 V385 в» ; U12588-’ QQ" Open Star Clusters and Asterisms kJ О to scale < S' Globular Star Clusters ф ® Ф to scale < 5' Planetary Nebulae -ф- <> -Ф- -Ф- >30" 30M0" 10"-5" <5" Bright & Dark Nebulae D a ° a to scale 10'-5' <5' Сг >5' to scale laxies О о о 5 -2 2-Г < Г major axis Galaxy Cluster •ч 'i to scale 00h52m to 23"08n +52° to +40° AND CAS IVrf Tinbrj / ferry Rappoport I WiN Rernuklub
31 +50° +48° +46° m V350 V422 V414 о U12088 V380 U12086 V407 12 DD о ”417 V418 U12125 .1 0 23 08m 23*04” ?,hftn 00m 22^” 22*52” 'S^7 +‘ v U1203. 7282 0 I M+746-9 U12204 xn. 44 22*40” 22*36” 22*32” 22*28” 22*24' +40° 28h16” ' 22/>l2"> /3*08” 23*04” 23h00m Г ./> 22 48m 22*44” 22*40” 22h36m • • • • • • ♦ • 1 • • • • 9 1 * • ♦ •• • • . • • • 1 • • 1 • • • ♦ V411 • m 22h24 -1 + LACERTA 1.5217 V382 U12433 о 7ф U1241] V379- U12341 U12381 . 16 EN I M+7-47-1 / ANDROMEDA ' U12095 /a V410 : EW • • • ' • * 1 • • • • • 1 • Pl 00.0-8.7 V421 О 5 (V412) V409 / • * • • 1 • • • • • jf - Л • • О ’ LACERTA ’• 22'>56m -22 1 • • •1 • • • • _• • 1 • ♦ • • • 1 • 1 • • • • —® — • ♦ • • • • V419 • • • • • • . R • © Amplitude 1.0 mag. or less ’U12057 Stellar Magnitudes (V) Double or Multiple Stars Variable Stars м Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" © ® © (•) ® © (•) ® о Amplitude Amplitude Amplitude 2.0 mag 3.0 mag. 4.0 mag and brighter 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright C 198/100! Willrrwnn-Bell. Im.
3 о 7086 LACERTA 80 Я' © AR +50° • нт .© 7209 LW V397 V394 В168 ©V2075 СМ I 891 V400 7197 2^44™ U11897 О I +40° 21^2^ U,18°6 U11802 оСХ 2200+420 r86^ % +53° <& 2,ь48~ 21b4-°”- 2'"W” h 4m 2» 4o 22h24m 22h20m 22h16m 22h12m 22h08m 22h04m______________22j)0_ +52° © । C1 ° • ’ V357®] • • • • • • • • • • • • •— +5 I +50° 4 • +49° • +48° i । A 7° 1.5217 •* ♦ 1 • • • • • • • • •L ♦ • • • • • • • • • • • • • • ♦ • • • • • • • • •• ‘ Cz.243 • • • • • • • 1711991° • ♦ ♦ • • > • • 4 'j- • +4/ • 2 • • • • ♦ • ♦ • • • • • oU +40 , A co • — • • ° FW ♦ ♦ • oV404 0 U11979 • < • • .. • • о 7231 • +45 • • • ♦ • • • • +44 1 +43° • i Л • • • • • • •• •- • • • * • • • V405 • © • • • • • • U11961 ♦ _ +4z о • • Ш197 • • S • 3 • V401 V402<* V407 о о Ш 2002 °C531-4 Р97.6-2.4 • * I “V2172 . В164 ваг2 p94.5-0-8 /V2165 +41° +40° 22h24m U12016 !_£___ 81 Я2 Х/2173 ° о 7250?248 ® • . UH920 • V365: • о UH909 НК U11911 ч ’ U11935 7223 * . U11927 RT BG • ’/ -..Сг470 Cocoon Nebula 0 *:5!<6« ‘ UH836 U11858 22^20" 22h16m 22h12m 22h0«m 22h°4™ 22h°®m 5 'Г U11805 U11_819_L о • Р933-2.4 I — —I •от * * х/2169 \Л339 © 7092 М 39 7093 •_ Р9Г6-4.8 • ®1S6 73 P " U11799 ^.gSS U11798 . -75-«Гии V2167. B1S8 Bl 59 В155 +45° +44" Open Star Clusters and Asterisms to scale < 5’ Globular Star Clusters ф ф Ф to scale < S' Planetary Nebulae >30’ 30"-10” 10"-5" <5" Bright & Dark Nebulae '/' □ l’j D : : to scale 10' -S' <5 Galaxies 0 1 ° ° ° >$' S 2' 2' Г <V Io scale major axis Galaxy Cluster to scale 21h32m to 23h16m +52° to +40° LAC CYG, AND IW hnon / Barry Rappoport! Will RemakJui
32 Copyright $ 1987 2001 WiUmann-Bell. Inc. ® ’ • V2139 Stellar Magnitudes (V) Double or Multiple Stars Variable Stars и Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" S ® ® © (•) ® ® (•) ® О Amplitude Amplitude Amplitude Amplitude 1.0 mag or less 2.0 mag. 3.0 mag. 4.0 mag.
+49° +48° +45° +42° +41° +50 +47° 20h48m +52° ,-- +48° 20ь04т 20h00m 19hS6^^0 20h44m 20h40m 20h36m 20h32m 20h28m 20h24m 20h20m 20Ибт 20 12 20 —_— О 3C418 26 e P84.9+4.4 Sh2- 2 V393 . • • Cr421 Do 6 M+7;4b1 DoDz 10 V2130 V2131 M+8-36-9 1 Г A0 vdB131 □ . Do 8 +43° • U11500 1111503 i 1.1318(d)} J '^6910 <Л\/2095 +44° p ) Л405 CYGNUS +40° I-------------------.J___ 20h48m 20h44m 20M0m 20h36m 20h32m */^3f8(t-)D° 1 ° 20h24 +40° —7"----- 70h00rn 19*56— 20h04m 20 UU 1° — • ♦ • • • ♦ • P88.7+4.6 < 51 • 0 • • 4 • • • • • • • • ♦ • • • • • • • • oV • • • A- • • ♦ • • • • • • • • V2126 • Be 90 • * • • • - • • • • ♦ -• CYGNUS C257-29 • Sh2-115 V2122® P86.1+5.4 ч§> 43 (V2121) /45 W’ (V2014) 55 (V1661) ♦ ' +46° 8350 V2132 Be 89 P84.2+1.0 8349 +44e>^ V2134 +43 1.5068 V2115 • ♦ • 32 О2 (VI488) K* '£i • . • • ‘ 31 O' (V695) V2109 °RX SV P84.0+9.5 C257-35 ; U115O7 1111499 +49° VI584 ® 8345 • • • • .30 • M+8-36-10* SW о a Ф V1773 50 (X Deneb • • • • • • • • • • Northern . Coolsack 8348 4729 CygX-3* Do 44. 8346 • Do 9 DW8 100-5-9 , : ^Olf LDN889 ; P78.9+0.7<+ . • oV2117 О • • . 1 • —I +45 ‘ \l.1318(b) ~'Sh2-108’- 8344 \------- m . .• 20*20— Do 43 -n Open Star Clusters and Asterisms Globular Star Clusters Planetary Nebulae Bright & Dark Nebulae to scale < 5' ® ф Ф to scale < 5' V" Ф -Ф- -Ф- >30“ 30"-10е I0--5" <5" □ □ i to scale 10'. 5 <5 _._0---- V2110 P79.9+6-4 6866 • © V395O P79.6+5.8 P78.6+5.2 + • Do 2 . 8342 1.1318(a)______L^- 20*36- 20^2"' 20*08- Galaxies to scale major axis Galaxy Cluster to scale о V420 ‘ \ Do 38 oV2098 19h56m to21h40 +52° to +40° m CYG IV.4 (non / Barry Rappafxjft / Will RemukJus
33 24 ||/ 20h04fn 20h00m I9h56m 19h m 19 48m 19h44m 19h40m 19h36m 19h32m 19h28m 19h24m 19h20m 19h16m 19h12™ —। +52 CYGNUS +5Г +50° +49° +48° +47° +44° f +43° ‘L +41° +42° V2O77" © RT V927 С25Л/7 +47’ FL° VI264 1420 RR C230-20; t/H446; . V476 V380 CYGNUS : LYRA 6819 . oV554 19h56™ 19^52™ +50’ +46’ ° C230-21 M+7-40-10 U11467 о ~ °u/1468 M+7-40-15 ° 0 U11464 ♦ • • • • • • ♦ 0 • • 26 e P84.0+9.5 Ul 1507 • ‘Uli 500 Ul1499 Uli 494 C257-19 +45° 6866 • VI675 Q 8-3 6-10 V2094 AXo^V2095 ’ V393 ° V2098 V420 " Do 3 6 Cygnus A M+7-41-J +40° 20\)4m AH,' 20h00m copyright C 1987 2001 WiWmonn №. »k Tvi 0' '°u"465 -Q- <16 • 0 j •• 6826! . ♦ .~U11485 •' Blinkin9 Planetary U11486 • 130 VI743 V2081 V2080<+> CH 1.4867— 01.1301 +49' 6833 +481 C257-16 Ul1480 • 1 • • • ♦ • • ♦ • • • • 1 <^V2083 18b • • • • • • • • • • • M+7-40-13 I °U11473 ------4-s— 19,’48m Stellar Magnitudes (V) S.5 6.0 6.5 7.0 7 5 8.0 8 5 9.0 9 5 9.7 V973 19h44m ® • V2087 • BR 6811 U11450 AF® aw P77.6+74.7 * 6783 Ul 1466 U11459 UV V2079 A2319 U11439 о U11430 о 6792 0 +45’ +44° +43’ +42° • RU • V552 +41’ 19h40m 19h36m 19h32m 19h28m 19h24m 19h20m 19h16m •+40’ 19h12m i Double or Multiple Stars Individual members are plotted if separation exceeds 60 Amplitude 1.0 mag or less Variable Stars Amplitude Amplitude 2.0 mag. Amplitude 4.0 mag. « Nova q Quasar Л Radio Source X X-Ray Source
3 +51° 6742 +48° LYRA +46’ +45° +44° С229-24 . +43° +42’ V552® +41’ m НК ®>oBY +49° +47’ +47’ ^8V'24rn . draco '8’'28” m 18W 18*52" 1.1291 V540 V548 М+7-39-14 М+7-39-11 LYRA Ф V543 18b24m • V550 <§> •« ’U11408 +42° +44° +40° •._______ 19h*2m 19h08m 19^04m 19h00m 18h56m 18h52m 18h48m U11319 6675 I 6663^ • _о___J——— 1йМ± 18h36m 18h44m 18n4U Л.4Е1 М+7-39-6-4 M+7-39-5. .о V547 6745 . ® о 6702 0 6703 r 3C388 U11357 I UH217 . » J +48° +50° +49° +52’ r'— CYGNUS • DRACO • о • • • • • • • • M+9-3M2 0 • • • о HP •• . • ° M+9- • • • • • 6764 4 • • o: ♦ • о 6759 • • • • • ♦ • • • • • • F • ♦ • • • • • • • • • • • • • • • » • •• • • • |-® • • 1 . • b • -I ^U113 76 • • М+8-34-33 U11406 ®V551 16 М+7-39-8 V541 .6711 о V538 1Л1298 U11329 М+9-30-23 М+8-34-2 3C38I U11287 V533® М+7-38-12 ЗС380 s М+8-34-1 с« 6672 • 1 1 \ • 1 • +50’ Uli 244 ♦ 1)11262 U11235 1.1289— ,sb32“ ,8>'28”’ +40 A8h20m Open Star Clusters and Asterisms / ) to scale < S’ Globular Star Clusters Ф © ® to scale < S’ Planetary Nebulae >30’ 30"-10’ 10’ 5’ <5" Bright & Dark Nebulae □ £ °[:] to scale IO1-S’ <5’ Galaxies 0 000 >5' 5'-2' 2-Г <1’ to scale major axis Galaxy Cluster to scale 18h20m to 20h04m +52° to +40° CYG LYR, DRA Wrf юг) / Buriy Hoppjport/ Will Retnoklus
78h28m h ИЖ *' 18 20 18h16m 18h12m 18h08m 18h04m 18h00m 17h56m 17h52m 17h48m 17h44me 17h40m__________________1 7h36™ М+9-30-9 DRACO Etamin 6466 о 30 +49 +45° +44° +43° +42° +41° 0 U10984 , UH241 0 +45° • 6478° +46° +48° +50° +52° +49° +47° +48° 6515 0938 OV986 U11112 6524 о V529 V566 Uli 190 LYRA Mi-7-37-33 90 f V522 18fl24m -36-30 +44° +43° +41° +47° UH 244 ♦ ' ° ° C254-21 6582 HERCULES . M+9-29-17 • M+9-29-16 6409 о +50° U11217 о Uli 202 AM Her oGX * V814 M+8-33-34 t •9 • UH206: ♦ © 88 (V744) z ’’I 6443 DRACO M+8-33-41 U11235 ° M+7-38-6 ° U11228 UH 204 : \\U11186 U11181 6606 UH 185 U11065 V984 HERCULES 82 y> ° C2S3-26 Ci 6560 © OP M+7-37-17 M+7-37-13 M+7-37-14 . M+ 7-37-21 ©V982 M+7-37-1 M+7-37-19 • M+7-37-18 M+7-37-4 M+7-37-10 +40° 18h28m M+7-37-34 • M+7-37-38*' * ' 18h20m 18h16m 18h12m м+7-: о • 7-20 ‘ о • • > • —• ♦ • • о • ♦ • • 18h08m 18h04m 18h00m V337 • • • • • • M+8-32-21 . V962 • M+7-36-31 U10946 * M+7-36-28 M+7-36-29 •Э • • • • • • • M+7-37 Cj ♦ • • -1 - • • • M+7-36-34 • • 17h56m 0 M+7-36-33 17h52m 17h48m V963 ] yh44m 1 7M0m 1.12651 +42° +40° 17h36m 6 0 6.5 Nova Quasar - 0.0 jndtXKjhie' ^ann-BeU. inc. AmplitodP Amplitude Amplitude 4 0 mag 3 0 mag 2.0 mag Double or Multiple Stars Variable Stars Radio Source Stellar Magnitudes (V) ~ I Amplitude individual members are plolt Q Qf |e$s IVlUUUi ------ if separation exceed bV X Ray Source
16ь56» ,6»»» '7h0° -- ' U10839 +51° 3C356 +50° +49° +48° +47 +46 +45° о +43° +42° M+7-35-50 +41° ...’6"" U10908 Q 1700+518 —о---- C253-17 1^2° +48° +49° +47° +50° 23 p ™ 17h28m 17h24m 17h20m 17h16m Rastaban < 17*36m 17h32m +52°---------------- M+9-27-69 ^ . M+9-27-68 HtRCUltSj +5V 'X/927 oV940 V792 3C352 0 M+8-32-5 U10845 M+7-36-4 • 6341 M 92 V9U 0820 M+7-35-56 M+7-36-6 0 M+7-36-11 о 6363 M+7-36-12* M+7-36-2 ’ 6339 M+7-35-61 6320 О M+7-35'13 i о 77 =0 M+7-35-62 M+7-34-146 . +42° M+7-3 HERCULES 0 M+7-36-8 +44° 6343 L/70812-^ О oTX 6350 ? 6348 Г M+7-35-53 M+7-35-33 V939o 6301 6312 U10765 о a U10759 0 U10710 о 6323 U Ю553 UM4m GQ .“/727+502 0 V952 U10806 U10814 82 у V953 +40° 1718+481 S’ M+8-31-44 M+7-36-7 +44° M+7-36-23 ° U263 I ° 11262 M+7-36-24 * \ • V957O • 1.1264 • M+7-36- 4 6-17 • M+7-36-/3 ъ • “V954 ‘ • • 1 • • • • DRACO ---••• P75.7+35.8 °6313 U10760 о 6336°| .6329 0-. V818 6332° 95 6327 M+7-35-58 0 M+7-35-47 —©V81? --------*Th,,m 17h36m 17h32m 17h28m 17*24m 17ll20m "6283 V925 U10571 6229 Ф* U10722 M+7-35-41 M+7-35-37 O 6311 . M+8-31,-19 .„о о o 6279 • ЗС349л M+8-31-2' 1)10681 M+7-35-17 M+7-35-29 M+7-35-30 M+7-35-36 ° U10627 ♦ 1)10651 V924 M+7-35-6 Ul061o о V923 V933 o6i41Zwicky'sTriPlet 1)10586 . U10531 6239 © V636 • о M+7-35-25 М+7-35-Ю U10707 M+7-35 -20 M+7-35-.19o0 M+7-35-18 V929 . о M+7-35-11^M+7;35’. M+7-35-12 . M+7-34-150 0 +40° . - 16*52* 36M8 —-J— о Ah56m ’° i7h04rn 17*00* 16 17h12* 17*08* I7 04 Open Star Clusters and Asterisms ()O о to scale < У Globular Star Clusters ® ® Ф to scale < 5‘ Planetary Nebulae -ф- -Ф- -Ф- ♦ >30” 30--10” 10--5" <5" Bright & Dark Nebulae <2?□ ° to scale 10’-5’ <5‘ Ge >y to scale laxies ooo 5-Z 2-Г <Г major axis Galaxy Cluster to scale 16h44m to 18h28m +52° to +40° HER DRA, LYR IVil Tition/ Bony Rnppafxirt / Will Reinakkn
„ m h,6™ 16412» 16* 16h°4"' 16h52m 16h48m 16h44m 16h40m 16h36m 16h32m 16h28m 16h24m 16.2° 16 T J t --------------,------------------—--- +48° +47° 0 +45° +44° +43° +42° +41° DRACO M+9-27-69 M+9-27-6S +51° +50° +49° 1/10571 6229 V921 52 624/ Q ° Zwicky's Triplet U10586 V913 о 1/7053/о jCi M+7-34-147 о 6239 M+7-34-146 • ® V636 . oV916 M+7-34-150 HERCULES M+8-30-26 • C251-36 42^V906 34 ° V449 I М+7-34-14 44.7 1Л. о M+7-34-12 , о U10511 M+9-27-58 • 0 M+8-30-10 M+8-30-35 1/10486 \ M+8-30-25 o'®0 M+8-30-24 0 6/54 C251-19 +48° +46° J. +45° +47’ M+8-30-27 _—------- M+9-27-50 M+8-30-39 ° i 1.1223 о EV U10168 M+8-30-20 ‘ V893 U10457 M+7-34-7 V905 A3 U10354 M+7-34-138 . M+7-34-/25 о !• o I 33-37 M+7-33-42 (JI 0200 . о M+8-29-31 ° 1.1221 ° 1.1222 M+7-34-123*3 M+7-34-140 (710480° --________•-----•---- . +43° 1 +49° +50’ M+7-34-/2S ° Л4+7-34-//9 M+7-34-120 Jm+7-34-117 “ M+7-34-116 . M+7-33-23 M+7-33.-24 о U10152 M+7-33-30 о U10357 16h16m 30g® 42197 М+7-33-2б\ . J +42’ М+7-34-/1/ ) • 35 6 "L/10396 1/10374 o. 6/55 3C337 O(J10437 ° M+9-27-26 M+7-34-32 о M+7-34-30 M+7-34-77 о • 6/59 U10430 . M+7-34-110° -26 UIMiSo„ kM.M4-52,SI6B« 1/10459 (J10427-"6,74 6)60 M+7-34-31-^6145 - --MT7T4-90 » л 4 -b ^-6147o6141 : a 6173-3^4^2,«1*6,46 M+7-34-92* T1,,, om+7-34-39 / 6184«^<,м+7.й.89 6^°\з m+7-34-27 М+7-34-97 «6)80 м+7-34-33' | М+Д34-47 - - . ' 'M+7-34;28 RR°f U1O278 0 42169 1)10156 ' oM+8-30-1 о 1/10325 U/0241 0 о nM+7-33-49 1/891 ° ?Д’к51 I M+7-33OI 6 V M+7-33-27 6058 +40° --- 16h52m о -° 1/10553 M+7-34-135Q -1/10512^- 16h44m M+7-34-62,61 J i 16h28m \16h24m 16h20n 42199', I6h12m 16h08m +44’ . M+7-33-25 +41’ (JI 0166 e +40° Л6+04->" 16ЬМ"’ 16h32m 16h48m 16h36m 16h40m Stellar yo Nova л 4 .0 mag 5.0 mag 0.0 0 5 jndb’MjbW COPTIC 19V-200' 2.0 mag- Variable Stars a Quasar 6.0 6.5 70 7.5 B.5 9.0 9.5 9.7 Double or Multip'e Stars Radio Source i .0 mag- bniphUid* X-Ray Source . $cpa<abO”
3! ithU"' 35bO^2° 15h36m 15h32m 3 5h28 3 5 _ М+9-25-52 BOOTES U10129 .Fl DRACO +51° HERCULES 47 V- +49° oST +48° +47° +46° +45° +44° +43° U10109 0 0 M+8-29-5 c> U10070 +48° ( +49° +50° +53° ^L//0097 +47° • о ' M+9'25'22 M+9-25-36 M^2%7I.1153 о H152 O U10118 '° M+8-29-31 M+9-25-33 5902 \ , +50° 1 ® tG FK M+8-28-4 U9936 0 U9997 1.1144 FO° ' 5918 © C221-50 0 5932 5933 M+7-33-3 4-' M+7-32-43 +44° Д +45° J M+7-32-4 \ +43° U9796V M+7-31'47 M+7-31-49 ? • 0 M+7-32-51 l"“4 M+7^S ' * \ M‘7f41 • 5900 О ® 96 -^4B 5895 5893 '5914A 1 и’Ч9 16h00m 15h56m 15h52m 15h48m 15h44m 1 +52° ---------------—r----------П—- M+8-29-13 Гм+8-28-31 M+8-29-4 M+8-28-37 M+8-29-8 U10010 0 1538+477 S M+8- M+9-25-45 0 M+8-28-.19 M+8-28-20 ’ _ M+8-28-28 M+8-28-3 о (J9835 U9761 +42° M+7-33-20 о C250-I8 ^M+8-29-18 M+8-29-12 M+7-33-M 4 (V839) . M+7J3-J5 M+7-33-18 d M+7-33-I6 U100"U10087 . о ° о M+7-33-6 M+7-33-11 U9924 U9815 О U9780 M+7-33-24 tw+7-33-23 +41° M+7-32-35 1 U9892O M+7-32-26 0 M+ 7-32-12 . 5935 jA r034 ,^4-5.945—Й934 5943o M 7.32.15 5947° ^M+/. U9873 1 M+7-32-22 U9840 +42° +40° 16h00m • M+7-33-19. 0______ 15h56m HERCULES 0 6013 . 5993 «5992 15h44m 54 ф 15h52m 15h48m M+7J2-44_ _ 15h40m 15h36m 53 V’ U9857 5929 . 5930 ° U9856 5923 -- о M+7-31-5? 5950 U9858 I5h32m 1Sh28m 15^20™ 5889 °o.c 5886 5888 M+7-31-39 M+7-31 -4° M+7'31'35 \ +43° о M+7-31'36 4' i5h"l 2m !5h36m 1Sb08m О Open Star Clusters and Asterisms to scale < 5 Globular Star Clusters Ф® ® to scale < 5' Planetary Nebulae -0- <>• <> < >30" 30"-10" 10'5’ <5" Bright & Dark Nebulae <2?<''? °°::: to scale 10 -5’ <5' G? Уо > S' to scale laxies ООО S'.2' 2'1 <r ma|or axis Galaxy Cluster to scale 15h08m to 16h52m +52° to +40° HER BOO, DRA WH Тиюп / Валу Rappapaa I Will Remaklui
14*28’’' 23 е зсзоз BOOTES EF М+9-25-33 5902 5673 1.1029 О +50° ° ЕС 5660 +49° 5622 +48° m О 5720 0 5624 о 1/9722 5689 5693 о> 5700 0^ 5682 5683 +45’ 14h52m 14h48m +43’ +48’ +49’ +44’ +51° М+9-25-22 • о (39702 М+9-24-26 * (39448 °- М+9-24-24 •О 5707 „ ° М+9-24-22 5676 о ® СИ 24 g \ М+8-26-31 I S М+9-25-36 44h40m 14h36m. 15h16m 15h12m 15h08m 15h04m +52° ---------------------- 39 -ЕТ 5633 1/9639 33 t/9780 ЕН" +44° U9598 М+7-31-13 О 1.1090 5860 (39542 (39684 +42° о 5630 (39641 М+7-31-35 (39441 +41° О 5772 М+7-31-36 42 [i ф Nekkar Uh28m д 4h40m 14h44m 5731 > 5730 5696 5697 1.1028 о 1/9796 +43° 5708 о U9386 о U9422 © U9314 <5 1444+407 Q U9429 о о М+7-30-43 кU9569 ° 1/9567 • о М+7-31-7 +46’ U969 Г О I - М+7-30-24 М+7-31-47 ) о • М+7-31-39 9 ° М+7-31-40 о °5784 5787 U9379 \ . о м+7-30-28 IU9376^__-i----- 14h36m 14h32m 139559 о BOOTES +40 ддЬ24т М+7-31-41 5900 ° . О *,3896 5899 ’ 58955898 5889 % 5888 ’ 5856 .о M056 М+8-27-52 М+8-27-62 5828 • 5о8'85797 5804 р к' 5805 о М+8-27-55 5835 I? М+8-27-60 0 М+8-27-43 (39665 °5830 ВХФ +47° +45° 5794 5795 о М+8-27-41 М+8-28-3 ° U9761 M+8-28-4 о М+9-24-35 +50’ 5767 27-27 ♦ M+8-27-28 38 h .0 М+8-27-40 ° М+8-27-31 1/9612 М+7-31-15 М+7-31-18 Г •’ М+7-31-218 '^м+7-31-17 М+7-31-29 ° EY" М+7-31-22 М+7-31-12 C22J-10 ? М+7-31-Ю » 1 • • 8 1,5721 5722 <717 М+7-30-54 0 5739 U9324 U9240 14h48m 14h52m 14h56m 15h00m 15h12m 15h04m 15h08m +40° --- 15h16m 5.0 L5 1^001 WHW"n‘8dl',’R 4.0 ^9 0.0 Cop/nq*” ® Nova AmpVitude ion*o or'e$ ^r. are plotted indivdua'^^^eO’ л separavon Variable Stars q Quasai Radio Source Double or Multiple Stars kmphiuoe AmpMwde X-Ray Source Stellar Mag1 initudes (V) 60 6.5 7 0 7.5 «0 Я 5 90 9 5 9.7 2.0 xomag
3( : URSA MAJOR 17 К1-2 23 0 211 +51 +50° • M+8-26-28 C247-15 +49° Al 904 o. U9211 о 3' о DU +48° +43° +44’ 5602 о о М+8-26-22 •Q> 5520 ,m 13*32^. U8639 IT 5250 1.902 0 5448 5256 5439 * U8588 L/8642 +45° U8611 U9105 +43° eCR 5214 о • о 5383 5320 U8651 BO 5410 U8726 M+7-28-71 5362 о М+7-28-78 о \38670 +45’ ’ М+7-29-27 BOOTES CANES VENATICI U8?17 5238 5225 14h24m +52° 13h44tn ^h40m 13h36 14h20m 14h16m 14h12m 14h08m 14h04m 14h00m 13h56rn 13h52m 13 48m U9178T BOOTES -A. 5481 do 5480 U9083 13 CF 1.95 J +50° +46° +44° +42° +41° 1 M+8-25-43 A 3C289 +48° +47° M+8-26-20 I U9I25 • ° . U9098 19Л 09056 __Q— 5500 о 0 U9068 5425 5377 • M+8-26-15 5391 ° U8876 DT 5608 3C299 I.U9216 56r°}n7^^98 ° M+7-29-62 5601 I +40° ^-922J йМ‘7'3°'1 14h24m 14h20m 14h16m DQ- U8798 о M+7-29-46 M+7-29-24 14h12m 14h08m 14h04m 14h00m Open Star Clusters Globular Star Clusters and Asterisms Planetary Nebulae to scale ) 85 П Alkaid U8702 5301 0 5297 й 5296 U8733 0. 5336 M+7-28-75 1)8756 о»?. о U8688 * M+7-28-64 5290 5289 „ ‘0 5355.5350 537 5358J&. U8841o sis3^4 ______________I 13h56m 13h52m 53B 13h48m М+8-25-18 +49’ 24 U8597q U8656 M+7-28-57 M+7-28-47 M+7-28-32 M+7-28-35 +40 l3h32m 13h44m 13h40m 13 3 Galaxies to scale to scale Galaxy Cluster О to scale о 2-Г 5-2- major axis >30" 30"-10" 1O'-5" <5- Bright & Dark Nebulae □ n □ i to scale 10 -5’ <5 IS1^" to ISMS'" +52° to +40° BOO CVN, UMA wr Гтоп / Bony Bappopon / W,H Remoklui
37 +48° +47° Н5°. +44° +43° +42° +41° 178651 +5'Г<0» -T--^ ,3h24m & I3b,2m ,зьО8,„ . U8222 — '4987 о СК 5250 +50 +49° № о ♦ о 178506 .24 ^5256 URSA MAIOR U8639 0 • М+9-22-20 5040 о 1-902 • 1 ..®/Р CWs VENATia'29 5195 Ь 5194 М 51 - ^Mrlpool Galaxy 1-4263 °Т - 5198 5173 M+8-24-108 ! М+8-24^о1 Jo I M+8-24-109 M+8-24-99 о 6R CI о • М+9-22-35 о 5009 О U8304 М+9-22-24 4998 М+8-24-68 U8272 13^04rn 13^00m 12^56m 12*152т 12*148г U8151 *4938 М+8-24-26 * М+8-24-36 М+8-24-40 । СС V U8597 0 ' I U8642 о, 178588 U861 ] 2Q аМ+8-25.17 U8162 0 4932 M+9-2 Л 1-68 • U8012 • 4707° • 3C277 • М+8-24-29 U8119* О М+8-24-14 О ’ 4837 ' +5 +4 °4741 о М+8-24-28 178331 io М+8-24-89 М+8-24-34гл ’ M+8-24-35^ Г J о I 5029 -4— _ . о 1 JY M+8-24 ]31 0 4917 • U8215 ° СО 178489 178327 AV 5023 О U8320 М+7-28-4 о 5145 о М+7-28-8 0 M+7-28-6 I X М+8-24-70 О 5021 о U8189 ° СЁ М+8-24-41 С-Ж 08225 М+8-24-56 ° M+8-24-4 b ” M+8-24-33 о М+8-24-86 М+7-27-24о CD. 4901 , А <5 ЗС280 °BQ ©ти ®BZ о 4800 +4 ЗС280.1 о 1.4060' 1.4100 О M+7-27-38 5003* M+7-27-28 ^M+7-27-26 M+7-27-34 О • ♦ • • • -• • • • Я" ♦ ♦ « • • • • • • • • м+ 4736 M 9 4704 °* 7-26-56 * • 4О • CANES 1 • 1.3850 * | 1.3810 0 VENATICI +4 +4 CN. oCR ° М+7-28.jg 5214 о о..', М+7-27-57 Sunflower Calaxy м+7-28-32 +40° I3^4om l3h36^ 73h 13h32m 13'128rri +4 ‘ ЗС285 178400 <л„ ' ™ U83'5 5055 М 63 о U8365 ° 19 СН 13h12m • 18 -M+7-27-45 ' M+7-27-46 M+7-27-56 20 AO .Ф 5093 23 13ll24m 13 20" 13h]6m Stellar Magnitudes (V) Double or Multiple Stars 4985^ 4963 +* +4 13h04m 13h00m 12h56m 12h52m 12M8a Variable Stars © ® © © © © (•) © © ®®O Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. п Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60’ o.o andbnghtw 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright V 198/-2001 WHImonn-MI. Inc.
37 М+9-20-77 о М+8-23-49 1)7560 U 74 08 U7910 4449 О U7577 1BV М+7-26-15 Chara 4655 р4157. 1° U7176 ° 4618 О о । М+7-262 1)7608 М+7-26-12 4485 3 4490 М+8-23-24 о М+8-23-69 U7690 0 V 4357 М+8-23-35 +49° +48° 4617 •о М+9-21-9 о -• A2h00m URSA MA\OR М+7-26-44 ь. М+7-26-43 4258 M 106т-i о. .®4232 4288 Q М+8-23-7 4460 Q U7617& о М+8-23-40 U7593 0 <2244-27 О М+8-23-67 BW° CANES VENATICI 1 I U7267 4b „ m ,242- '2bM” ----1 о M+9-20-153 \ M+9-20-172 О U7082 A1452 65 ON О °4051 1/7340 +40 М+7-26-7 I +44° +50“ 12h00m UW” ’г"04 „Ыб"' ’2"’2 !2h20m 12 16 Q 4242 . °U7416 O Bl) 12h48m 12h44m 12h40m 12h36m 12h32m12h28 +52° +51° +50° и’ U7950 о М+9-21-42 ° М+9-21-43 М+9-21-46 • • • • oM+9-21-1 • • M+9-20-156 О • 9.4537 ^ 4542 • • M+8-23-29 —i-BT_ __ 1 • • +49° М+8-23-80 11 +48° +46° +44° М+7-26-27 +43° +45° +47° 4704 вх 4625 о < +41° /.3713 о 13726 °I3783 CANES VENATICI +40° --- 12h48m U6922 4187^ М+9-20-116 4088 1 4085 О ♦ о HZ U6992 О о U7367 U7358 4218 4220 ° L/7823 1/7639 4346 42261 о U7325 М+8-23-65 М+8-23-61 о M+8-23-51 М+8'2^М+8-23^5 М+8-23-32 4392 4389 ° UY i и7525« М+8-23-31 I t.U7444 U7486 ЗС272 А U7774 —— . 12h44m !2h40m 12h36m 12h32m 12h28m 12 2 М+7-25-57 О 4100 4047 U6930 3985 4096 • о М+8-22 М+8-22-80 _ м+8-22-76 9-м+8-22-73 - М+8-22-84 URSA MA|0R 4137 о 4001 -54 о 4010 H\N М+7-25-12 о 4013 4183 О OU7271 4135 • 4138^3^268.4 о 4117 М+7-25-47 41 18 '41П 4109 67 1.749 о 1.751 4143о 0В5 1/7129 { М+7-25-31 о С215-50 Open Star Clusters and Asterisms 00 О to scale < 5' Globular Star Clusters фФ Ф to scale < S' Planetary Nebulae о >30" 30" 10" 10’5’ <5" Bright & Dark Nebulae to scale 10 -5' <5‘ Ga >5' to scale laxies О о о 5 -2 2 -Г < Г major axis Galaxy Cluster to scale 11 h56m to 13h40m +52° to +40° CVN UMA WH Jtnon / Barry Rappoport i Writ Remakkn
38 +5^604m U7082 Al 468 +51° ^+9-20-77 о U6667 llh44m Тз9ЪОи680^ ‘ °M+9-19-97 ° U6555 I ’ ! 1176Я1У I • ' M+9-,9-'67 ^ /"67ss I 176811 I 12^0()т Ur^A^MAJOR Al 452 i ’ - -% Jlh32™ 1P\28m 11^2401 1Jh20m цК^т I ~T ----------------Г------ — ------------------- +52° о 176505 +50° +49° 4026 U69S6J 0 U6922 176992 • 1 M+9-19-57 I.°? IА1218 13+9-19-53 Arp's Galaxy ° U6i09 M+9-19-68 — — ----------- — U6399О о M+9-19-51 +51’ 3924 *3922 0 3870 <2/ 176917 о 1.705 13+8-21-88 Mi-8-22-13 • W,3 0 U693Q &3C266 ° 176726 ° I 1731 I 17654 1712 7ЛО M+8-21-46 I • . 'M+8-21-67 113+8-21-69 < i 13+8-21-72 _M+8-21-74 ° 4047 ° U6713 J-709 L I 7ll M+8-21-45 A1314" +48° 3985 ъ W0.3 3949 Mln^ure Spiral P 3893 3932 QI 3896 0| 0 HT 3906 I I 0 W+8-21-93 63 z Q> U6380 +50’ HP 0 Mi-8-21-39 3583 3577 +49’ '3769 5> 3769A 176576 • U6606 • 1 3726 • • 60 M+8-21-61 • M+8-21-44 ' 3782 • • ®EE 3677 M+8-21-38 M+8-21-37 М+8-22-54 °HV М+8-21-58 0 3811 3877 О ° 4001 4010 M+8-21-90 * 0 I ° Mi-8-21-92 ' ? 13+8-22-21 85 DM . ' + 3741 13+8-22-32 I М+8-21-42 +44° M+7-25 0 ° .1 M+8-21-75 176818 U6628 • ®5Т о 1.687 U6410 < ® +48’ +42° M+8-21-16 I ° М+8-21-13 0 Mi-8-21-12 3614 Q 3614 A 1)6255 Q 3595 +47’ +46’ <• Mi-8-21-2 0 +45° 3938 о' U6776 0 I 4013 +31° Lq /. 173020 М+7-24-16 M+7-24-5 0 М+7-24-23 +43° 59 • 58 0 3675 +40° 12 h()4m o 176865 U6901 , M+7-24-27 U6611 I 0 I M+7-24-21 13+7-24-29 1-750 щ49 / 0 1-751 U6529 12"Оот 11h52m 11h48m 111144т 1 lh40m llh36m Stellar Magnitudes (V) 52 VI +44’ U6266 +43’ 176805 U6489 М+7-24-10 1121+422 P 3600 3C254 <S) +42’ M+7-23-32 ___s +41’ 11632m 11h28m U6455 1lh24m Double or Multiple Stars Variable Stars ° M+7-23-40 URSA MAJOR 11h20m 11h16m +40’ 11h12m Amplitude Amplitude Amplitude Amplitude 1.0 maq. or less 2.0 maq. 3.0 maq. 4.0 mag. Q A X Nova Quasar Radio Source X-Ray Source Individual members are plotted if separation exceeds 60" 0.0 andbngM* 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright © 1987-2001 Willmann-Bell. Inc
38 • U5928 • HI wv U6162 О +50 +49° +48° U6227 +47° C24J-36 . U6201 -56 M+8-20-38 U6015 U6075 ’M+8-21-1 U6187& +45° GW- 52 V 1 U5953 C241-60 +44° 0 +43’ +42’ M+9-18 C241-13 M+8-20-89 О 0 3191 U6101 о М+8-20-77 U6135 о C241-74 +49’ +48’ нм +42° о ° 06103 U6125_____ +47’ +46° U6129 U6131 __и <=> М+8-2С О 3478 U6076 ж. М+7-23-32 +41°° — 3406 *3410 М+9-18-72 о U6013 OU5991 М+8-20-92. е> 0 М+8-20-32 ° U5917 А о М+8-20-45 U6038 ^06071 ~ М+8-20-61 U6127 о U6205 М+8-20-87 ° U616S* U6136 —0“*-----------7 U6106O U6100,. inh.Qm юЬлдш Ю^АО’11 1lh12m 11 h08m 11 h04m 11 h00m 10h56m 10h52tn_________________——— +52’ -------- ------- T~----------1----Г <=> 3298 0 3320 U5714 U5744 U5604 3198 TX® U5698 U5845 3202 U5941 M+7-22-29 • о U5838 3468 M+7-22-25 10h24m .M+7-22-46* о U5996 ° 47 Wh28m Wh32m M+7-22-60 10h36m URSA MAJOR 10h44m 10h48m 10h52m 10h56m 11l'00m 11 h04m 11h08m М+7-22-44 3Oh4Om +44’ +50° , М+7-23-19 Mayall's Object ‘ о U5740 U5754 +51 O • • 1/6232 о 1.674 +40’ ---- 11 hl 2т ]*U6074 о U61 , n M+9-18-69 4 U6008 • U6 09 1 i X 4 US998 ° « 1 ♦ U61 'о M+8-20-71 ,• C241-15 U616J M+7-23-18 U6149 M+7-23-9 M+7-23-10 3C247 0 M+7-23-15 24 M+8-20 115872° . U56O5 M+8-20-31 M+8-20-24 M+8-20-22 M+8-20-18 U5798 C241-2 M+8-19-39 o U5746 3416 0 3415 45(0 • M+7-22 41 • -59 Q U5859 M+7-22-21 M+7-23-3 M+7-23-1 ® to М+7-22-34 О 1)5771 M+7-22-22 M+7-22-27 3319 M+7-22.-H . M+7-22-12 0 U5707 U5657 ,oM+7-22-10 Al 035 +40’ 10ь20п' Open Star Clusters and Asterisms О О о to scale < 5’ Globular Star Clusters Ф © ® to scale < 5' Planetary Nebulae Л V < >30" 30--10" 10' 5' <5" Bright & Dark Nebulae □ LJ O : to scale 10’-5‘ <5* Ga 2^0 >5 to scale laxies OOo 5-2’ 2'-Г <Г major axis Galaxy Cluster \ J to scale 10h20m to 12h04,n +52° to +40° UMA WH Ttncm / Harry Happaport / Will Remoklu^
39 +51° +49° +48° +41° m » 09h56m 09h52m ^8" ^24. U5460 +42° US3S6 @31 SY US3S4 М+8-18-29 М+8-19-8 ЗС239 US237 U5368 •° М+8-18-57 О °C21i-i4 3184 3179 О М+7-21-Х © ’ US 87 3104 LE0 minor 10h24m US476 10^2Qm 1-598 о О — 3135 • 3111 US4S1~ о M+8 -18-64 M+8-18-32 M+8-18-33? M+8-18-40 M+8-18-62 ----Г ° M+8-/8-S6 cm <s>. J оМ+8-lf.i, 9 US290 U5295 М+7-20-72 • 1 • • • • 1 1 +43° I. 7 0^2 gm U5S4S Abridge 1618 ? US6S7 (75605 (75604 ° 3191 ^^+8-29-32 M+8-19.3s 3207 3205 3198 0 С240-22 М+8-18-60 о M+8-I8-S9 • m • • • URS A MAJOR • ♦ • • • • ♦ • t .. • • • * • • M+8-l< 8-23 +50с +49' 6m +52 +51 US172^ M+8-18-16 * 1/5145 1/5151° о M+8- 8-2S —-----------•- +48 о M+8-18-1 M+8-18-12 ;M+8‘ US1S7 о ——— —- о M+8-18-42 M+8-18-3 4 U5169 • • 0 M+8-18-. • • • U5225 i5 • • • ♦ • • • +47 +46 ?да 33 Л W^ldf+i Stellar Magnitudes (V) 4C+41.21 <S 1 ohl 2m US199L 0 М+7-21-2 ' 19 10h08m 2? M+ 7-20-37 M+7-20-40 LYNX 10h04m 10h00m 09fl56m 09h52m U5133 о M+7-20 ’ M+7-2 3°,03009 67 0-66 .300S 3008 -% 2998 i a M+7-20-S7 M+7-20-68 • • • M+7-20-S8 ♦ Oo +45’ +44' U5135 ^M+7-20-30 ----1—ТГ- -r. . +43' M+7-20-27 M+7-20-26 0.0 ' andbughte 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 6 0 6 5 7 0 7.5 8.0 8 5 90 95 97 • • Double or Multiple Stars Individual members are plotted if separation exceeds 60' 09l’48rn Variable Stars M+7-20-33 ? US 198 0 M+7-20-32 09h44m 0 I M+7-20-2S +42 +41 42 -о М+7-20-31 09h40m +40 09h36m Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag 4 0 mag. M Nova Q Quasar Д Radio Source X X-Ray Source Copyright + 1987-2001 Willmann-Bdl, inc.
39 +48° +47° +45° +43° +42° +41° +52° г—09h28m 09h24m 09h20m 09h16m 09h12m 09h08m 09h04m M+9-16-29 0^076 +51° +50° o I M+9-16-22 +49° М+9-16-30 ъ 25 0 . о U5047 2841 9 М+9-16-8 М+9-15-118 RT M+9-I5-J11 о 04932 о M+8-17-87 C26S-17, Й • (l 0 M+8-17-109 Gl о • 2882O 2856^, ♦ 2854 • • • M+8-17-110 0 • • 1)4958 о • • 9 М+8-17-103 • ° M+8-18-7 . U5090 +46° 0 05026 +44° • U5091 Q> e © ♦ • 05045 c M+8- 7-102 о М+7-20-11 M+8-17-84 д 3C219 о 04982 U4927 M+8 M+8-17-69 U4930 -17-70 U4917 U4922 о BE • M+7-20-20 0 I M+7-20-19 URSA MAJOR LYNX +40° _____ 09hJ6m 09h32m М+7-20-4 о a 2860 о М+7-19-67 М+7-20-1 М+7-20-2 М+7-20-6 I BF • 2852^ ° °2844 М+7-20-9 о 09h28m 09h24m 09h0(F 08*56^ 08Ь5^_ 08h48^_ _08М4^?о URSA MAJOR 15 f U4717 . DH M+8-17-9 M+8-17-35 M+8-17-34 M+8-17-27 । A757 M+7-19-22 2755 о 2693 & 2694 2681 О U4628 04765 о 0906+484 Q 04753 °U4824 +48° +49° M+9-15-52^ +51° М+8-17-40 * о 04778 • о 0846+513 . 2739 © • 2740 о 04749 1/4551 FR U4580 U4598 M+7-19-21 U4556 Q 3C216 04805 0 04798 +42° +44° +43° 04649 Р 04635 ° о I М+7-18-59 * М+7-18-50 ИГ 2769 2767 ff^2762 2771 М+8-17-48 о 04812 M+8-17-55' 0 U4844 Q 04874 * 04868 о 04870 • -.U4829 о U4784 U4719 Talitha M+8-17-14 12K 2639\° +50° U4587 ! о U4892 U4919 . 2776^ U4881 : М+7-19-57 4-Q_______L oM+7-19-51 • 36 04882 ° М+7-19-37 ° M+ 7-19-44 M+7-19-46 2799X^4904 .M+7-19-50 2798 ° 278 ;5 о о U4867 . U4872 ^ 2782 09h20m 09h16m 09h12m M+7-19-31 о M+7-19-20 . M+7-19-30 • 09h08m 268 7К, В. 766 * 2686В- 9V ° U4709 °2712 U4686 U4700 U4659 U4648 ' M+7-19-14 M+7-19-13 09h04m 09h00m 2676 (J4562 C237-18 C237-21 FQ LYNX +45 М+7-18-63 о ’ 04642 • • • • • M+7-18-52 U46c2U4609\ ° г (J4578 о M+7-18-45 М+7-18-55 RS7^ ° М+7-18-54 М+7- о'^ М+7-18-44 О 08h56m 08h52m 08h48m +40° 08h44m Galaxy Cluster to scale 2-v < major axis UMA LYN, LMI / Barry Hoppapoa / Wl„ Remak)ui Gpen Star Clusters and Asterisms О c to scale < s' Globular Star Clusters I Planetary Nebulae Bright & Dark Nebulae Galaxies to scale >30" 3040" 10"-5" <5- -^5 u L.J О to scale 1(y.5. 08h44m to 10h28m +52° to +40°
40 URsA МА/or 08h4gm no, O8'M4m^ 0gh4()ni ^4546 7" 08h36m 08h32m *** 08 24" 08^20" 0846" 08h12" 08^08" 08h04" 08h00m +52' «4499 LYNX +50° +49° FR +48° ° 2676 ^+8-16-23 CW M+7-17-30 M+7-18-17 ° «4426 о M+7-18-2 «4628 ^846+5ji +51° ® • °2639 CP 04136 ) M+^8-57 8-55 ' +40° M+7-l8.54 «8<152П7 ^зв7 V4S!' +50° +49° +48' +47' «4543 +46° +45° +44° L. .SZ 35 +44° +43° L. • 28 +43° «4609 +42° SW 04188 «4635 +41' ° 04176 OSKAS'71 ®TZ 08<,44m LYNX 08h32m 08h28" 08h24m U4252 о «4578 О M+7-18-4$ 04148r V 0 U4463 «4449 +51° M+8-15-35 M+7-'8-50 ' J--------------- ^+7-18-44 M+7-’8' ^+7-18-37 1/4226 04200 M+7-17-12 0 0 «4580 «4562 «4525 • •ss 27 FO0 M+8-16-8 2552 • —H ♦ < 025/8 • • • • • • 2500 ’ 04309 о LYNX я / M+8-16-19 ^+8-16-22 за 97.1 2541 3C196 04258 о 04260 04209 «4393 M+8-15-561 '2537 о U4250 2537A Bear Pow Galaxy 0 ' • . 1-2233 M+7-18-39 +42°eL^/W+z’z^ «4598 CR о 4-^<8-i/ 1. 931 • 1 1 1 • M+7-17-24 ^+7-18-26° M+ 7-18-23° I «4513 1—-----a «4498 08<l40m u 08h36m Stellar Magnitudes (V) за 94 M+7-18-1 M+7-18-5 08h20" Double or Multiple Stars M+7-17-23 M+7 -17-26 08h16" 08h12" Variable Stars Amplitude Amplitude Amplitude 1 0 mag or less 2.0 mag. 3.0 maq. 08h08" 08h04m --- +40° 08h00" и Nova •) © о S Quasar Amplitude A Radio Source 4.0 mag. X X-Ray Source Individual members are plotted it separation exceeds 60" 0.0 and brighter 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 (.opyryhl C> 198/-2001 Willmann-Bfll. Inc.
4( »Lh»Tw ?NX \fo 08honm +52° +48’ +51’ +50’ +49’ O^O” 07h48m 07h44nl 07h40m_ «2 — • • • ’ U4071 . • • A595 '-' • • М+9- • 0 М+9-13-47 13-56 о О U3963 • ♦ • • ♦ —•- • • • U3973 О Э°1471 • 4-34 0 ‘ м >♦ • o|°M+8-14-3( +8-14-32 ♦ ° 1 1 2 • I л . • 1 —" 1 • 1 • 1 • • M+8-/5-32. 0 • • и U4070J • о • • 1052 $ M+8-15-5 U4051 • • • • U4107 л • U4082 • • • • • • 1.472 М+8- • • • • • • • • • • • ’ о • . U4007 -CD • • • 0 ® U3949 • • ' UY • ,® O U3792 . • . • 1 • U3684 o\ J +51° М+8-13-Ю2 Oy32 . 4 2326A\ о 1' 2332 V M^T^fehV3j-^e -"C2 34-105 ’o ^*3725 . M+8-13-106 • +47’ +46° ?U4136 ♦ 20 BZ • U3863 • 26 '• *25 +47’ U3831 • 21 1)3812 „м+8-l4'6 BY 2344 о U4056 Cl U3933 66 U3976 U3997 1/3966 MX. U3860 . U378J •*64 ' +4V o M+7-15-15 +49’ „10? M+8'13'9 M+8-13'1X_ RS , 2329 ^M+8-13-61 U3696 м+8-13'72 AS69 J3724' +48° 0 1)3706 oBM U3845 M+8-14-38 C236-13 U4000 о о ♦ • • • • . 1. .1 • • • • • • • • ♦ \ е ’ OU38JZ 1 Д-—*— 1 — 1 • 1 • . 0WOO8 • • • • • • • • • • е • • 1 • • • • Г auriga_ ___—V—— • • X 1 <2206-29 0 • • • • • •; ’ U3844 U4087 +45’ +43°. +41’ U4148 0 +42’ +44’ M+8-15-26 t> M+8-15-24 M+7- 7-5 U4018 LYNX U4068 М+7-16-Ю U3871 U3825 2337 о @V463 +40°---------------------- —— ---------- — 08h00m 07*56" 07*5,2" 07h48m +40° m 07* 07*42" U 07*20- 07M6 _________________ h oW 07*28" 07*24" " & 07*40" 07*36" °7 Open Star Clusters and Asterisms f Л Г Д C) (0 scale < 5’ Globular Star Clusters to scale < S’ Planetary Nebulae -ф- -ф- -Ф- * >30" 30’-10" 10"-5" <5" Bright & Dark Nebulae □ ° - to scale 10‘-S’ <5* Ga 2^0 > S’ to scale laxies О о о 5 2' 21' <Г major axis Galaxy Cluster Z “ s to scale 07h08m to 08h52m +52° to +40° LYN AUR, UM A WJ Tinon / Burry Ruppupurt I Witt Rcmokkti
41 LYNX +5/° AURIGA 0 U3477 +49° 46 l|f® +48° \7460 • M+8-12-33 '° U3506 * U3467 . M+8- J 2-24 о O7nogm <33645 +51° +50° +49° +48° +47° <33614 lynx ®Y463 +43° +42° +41° M+7-IS-4 о <33592 133487 _____^M+7-14-15 133481 ° +46° +45° W25O +40° °2hl6m n °7hl2m _7, <’7 08” 07*04» №510 о . ~ -S2\^ 06h40m* U3593 io M+7-15-2 4569 07h°0m o6h56m 06h52m -e* - °6 44"1 06h36m 06h32m 06h28- 06^24" ‘ * * +52° (J37S8 M+8-13-102 I ° • d c М+8-13-109- . 3 J 1.465U 2 +50° O2340^a C234-1O5 • 3-106° f<22225 М+8-13-ЮС M+8-13.9] 2344° 2322 M+8-13-46 о <33638 ,,, 2^9'1 ^8.13.59 696 %Л,М+8-13-61 \ M+8-13-72 M+8-13.74 ®NY О C260-37 U3568 • - • U3576 • • • • • / ~^356!~J • о ♦ • <3234-31 U3567 U3597 (33608 *v<62 O’ <3234-39 ' О 0 16 o <73588 a”V6. <33538 Mi-8-13-8 .V461_ o . 0642+449 • '• * • U3SS4 1 0 < — - • Г133535 1 ^0353, • 56 l|/s • • • • i 1 • ♦ • 4 50 • ° • • 58 n/7~~ • • __ U3512 I • • —s • • • • M+7-14-19 2281 07^00m u^01-— “h5°" 00*40» 06*44» Stellar Magnitudes (V) Double or Multiple Stars ° U3493 V457 • 47 AG +44° ~ — ------- -------.i_J— ____+40° 06h36m 06h32m 06h28m ’ 06h24m Variable Stars • ® @ ® ® (•) © ® (•)<•) Q Amplitude 3 0 mag Amplitude 4 0 mag в Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" Amplitude Amplitude 1.0 mag. or less 2 0 mag udbf^ttf 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright © 1987 2001 Willmann 8dl. Inc
4 Rs U3 375 ADR U3346 +50° 41 4553 +47° +9-11 2165 +48° +49° *+51° +50° £6^h20m 06h16m 06h12m 06h08m 06h04m 06h00m 05h56m 05h52m 05h48m 05h44nl 05 40 +52 o 2208 V446 -----• ©V439 U3418 V443 RR о ® QR M+ 7-13-3 05h36m 06h20m 05h48m 06h16m 05h52m 06hl 2m 05h56m +44° +41° 05h44m 05h40rT' 06h24m +52° +51° C259-8 O U3355 C233-11 ,KQ ' 2126 • 27 0 3C147 GA OC258-1° C258-9 tr 46 \|f’ • • +49° • +48° +46° +45° +44° +43 +42° +41° L— 3C153 M+8-12-9 V403 М+8-11-12 @ 36 (V444) . M+8-1H0. M+8-12-18 C203-6 e*42 43 C233-2 V449 U3407 • V447o •SV •RS &U3374 39 °V445 Menkalinan U3369о • I • I • < • • +45 +43° +42° ®V430 AURIGA +40° 06h24m 06h08m 06h04m 06h00m +40° 05h32m to scale Open Star Clusters and Asterisms Globular Star Clusters Ш W Ф to scale < 5' Planetary Nebulae Bright & Dark Nebulae Galaxies Galaxy Cluster 1 >30" 30--10" IO"-5" to scale 5-2 2,|' < major axis _J 4 < L—I L-J □ Io scale I0.5. >$• to scalp 05h32m to 07h16m +52° to +40° AUR LYN Ппоп / Barry Rappoport; w>H Remaklui
42 05^40m 05^36m к KM «« 0-$h28m 05h24m 05h20m 05h16m 1790 ' 05h08m 05h04m 05h00m 04h56m 04h52m °C258-1 9 (V398) +50° +49° +48° о +44° +43° +42° +41° о C258-10 C258-9 +42° +48“ +49” +50° +41° U3260 04h48m ------ 4-52 PERSEUS +51° V594 их 1724 1798 М 1 з а В? 15 V412 V407 AURGA RX 10 T) S BF +45° +44° +43° +40° 05h4()m 05h36m 05h28m 05h24m 05h20m 05h16m 05h12m 05h08m 05h04m AURIGA |ДЗС/37 oV421 М+8-10-1 М+8-10-7 V418 .ВК 1883 Capella V408 • Be 14 Skiff/0458.2+4301 Sh2-224 Be 70 V425 20 р PU SY V430 U332S ’ Сг62 • • •> • • • 0 . V415 1 • • • • • <15X • • *4416 °uz ’ • oV414 & • • • • • • B25 г • • I • • • , : -j ; • • .+46' Р163.1-0.8 ЗС729 1664 • KS® V593- —J +40° °05h00m 04h56m 04h52m 04 48 Stellar Magnitudes (V) Amplitude 2.0 mag Individual membets are if separation exceeds 60 X-Ray Source °0 ns 1.0 jndbnghw Copy«,h,r^«’'W1"mo,'"eC"-"K Nova Quasar Double or Multiple Stars Variable Stars Radio Source Amplitude 1,0 mag. of less VS "SS 50 5.5 60 65 70 7.5 8.0 8.5 9.0 9.5 9.7
Open Star Clusters and Asterisms to scale < 5' Globular Star Clusters to scale < S' Planetary Nebulae -ф- -ф- < >30" 30"-10" 10’-5" < 5" Bright & Dark Nebulae ° °::: to scale 10 -5' <5* Ga ^0 >5' to scale laxies О о о 5-2 2 -Г < Г major axis Galaxy Cluster *ч 'i to scale 03h56m to 05h40m +52° to +40° PER AUR Wi/ 1нюп / Buriy Hupfxipua I Will Remoklus
43 +4J° P3hO4m o4h00„ 03/Ч8П. 0Jh4,m “З'ЧО"’ 031>36” 03132» 03jW»_03h24» 03120” I. PERSEUS' King 7 ’+51° +50° 49° +48° 47° +42° +50° 43 34 V575 +49° *>'Q 39 S +48° 1245 +47° V577 +46° +45° 27 К U2596 0 . 30 32 I +43° U2723 U2700 & 1334 U2612 ol335 U2859 U2798 ’AB U2654 о * 02640 U2655 * C540-79 1250 +44° М+7-7-7/ 03h16m O3h12m +52° о U2598 о C540-59 —------ +41° ’U2618°l}01 . ^^608 +42« U2775 I o I 1 M+7-8-13 1/2674 04 C540.^2 1° ';4° U27 7 о <^U271o\ £• 'U2708 U 2 617-. — 1 И.309 U2689 U2686 ,’ * -U2659 ♦ +440 - +434 P149.7-3.3 ° U2851 • U2844 U2849 • M+,7-9.1 о U29M * M+7-8-35 V376 O-VS8Q PERSEUS +40° . «с 04^ • O4”oom w л , M«” <№s2„ ... °348" »3fc«» Mel2° | 1348 ©37 у . V396 U2773 c * 35 n V578 V576 • P149.4-9.2 a Nova Persei CK-N1901 ; | V572 < • • • • 29 • • 31 V410 • • 1 »• U2837 ® M+7-8-25 03^36- M+7-8-20 -U2756 .= «с, U2766 U2752 9 1727364 -f' M+7-8-4 1.316----------- ' ° • | ’A426 ’ I Perseus Cluster 1275 Perseus л .Ж ‘ I ! I 1293R 1294 M 12711260 128202673 1 © V510 1265 °o^2 * 1264 о i <3 .. Aq 'о 160 1.310 1259 • 1.311 J - • --------------------- +40° 03h24m 03h20m 03h16m 03h12m 28 CO Stellar Magnitudes (V) 0 5 1.0 1.5 20 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars • • • Individual members are plotted it separation exceeds 60" Variable Stars О ® ® (f) ® © (•) ® ® (•) ® 0 Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. « Nova Q Quasar A Radio Source X X-Ray Source Copyright ^>1987-2001 Willmonn Bell. Inc.
02624^ 02h20^2o 7''\erseus \ ГоЦ2380 PERSEUS ANDROMEDA +51°. AY' Mel 20 +50° V566 • +49° 62 c +48 +46° +45° m Q2h32m02h28m +48° • n jp U2261 U2270° P141.7-7.8 U1930 О ' / RR' +47° +49° +47’ VS52 \ 1 +53° •63P2. ® ' Tso° 03h12m 03h08m 03h04m 03h00m O2h56m 02h52m_________________ +52° М+8а5-5 65 H39 U2459 V570 о U2449 U2537 их (12043 M+7-5-43 956 U2573 U2233 27 К 1193 ‘ U1830 1160?. 1161 U1867 O1169 °U2504 .. J +44° +45° . ° <2564-17 ® V509 U2240 0 oRY +44° A4 +43° -‘-ту U2559 о 1186 1.288 • 66 ' U1957 oC554-16 U2351 °U2314 V5S9 1.257 0(12317 U2249 V561 о 920 b117l AE • 1159 U2470^9^ U2269 V557® . U2342о 1138 U2035 (12196;.*, ' ^558 ; 14* ♦ v’ul827 U2161 о U2227 о C539-37 o' U1987 “2!72 Ui« \ OF +42° -4568 A426\- Perseus Cluster \° .-.1224 ' о < 1.293 1177 , 0 9 1284, 7775 ° 1164 C540-19 +41° 1325380 ° 1198 о U2528 о ’ U2534 U2500 0 U2495 Л о *. U2473 ° 1.292 ' о 1.294 . PERSEUS ii_______ Algol (Demon Star) • V568 U2463 +40° __________ 03h12m 03h08m 03h04m 03h00m M+7-7-1,. i U2370cj9 1.262 P144.3-15.5 J1039 M 34 0 • . . U2101 ° U21 75'- '• 1.266 О Mj+7-7-_7_..»l — OU2361 1.265 Ц30 | U23SO J’22 •OU2280 • A372 о 1106 , _ . ’«M+7-6-74 U,85,'j,8i7»?J>2.b«‘ 7 uSf “У7!5'42 J,8S9 tKjern»"1 ( ^8” i • 946 937 \ / "909 906 • ’ ° ° 914° -V"' ’‘.923 и cP.-Ul 66 V M+7*y9,^lX858. ’M45'39 Д347 ‘ U184°. J.U19H—-V'" . „ oUlfBS .= )„6 1 , +— , M+7-6-18 a T . • Д°и1989” U2074 ’ m+7-6-34 ' elu2°73 I \ • (J2001 о I .. * U2215 "7 М+Л6^ 999 <->и2111 1, - jooi^M9^ o 1053 1005о'ь°9^ * O • 1 1000 U2194 • ’ . . Д *2 Ц2]86_ Д_Д-'—- . i обзo'; 0 U2060 <2 980 ^982 •°U2034 o U1988 0 U2185 V377^ (12277 ° . • ’ .• • ° U2256 I1077A 1077B P U2126 12 ( - . лэЬлдпп 02^40^ ^ 021-52» 02"48" »2« J +42° , +4V 3C65 +40’ m 02b20tn 02-28- 0244 огь^ о2”52" Open Star Clusters and Asterisms О О О to scale < 5' Globular Star Clusters фф © to scale < 5' Planetary Nebulae -ф- -0- -Ф- >30" 30--10" 10--5’ <5" Bright & Dark Nebulae <C2<j □° to scale 10 -5’ <5' Galaxies 0 ° ° ° > 5’ 5 -2’ 2 -Г < Г to scale ' major axis Galaxy Cluster ’.71 to scale Ог^О" to 04h04m +52° to +40° PER AND Wd Гтоп / Barry Rappoport / Will Remoklui
44 02h28m 02h24m +52° RRo +51° iZ Р130.3-П7 +49° +48° +45° 01692 m m m 01h48m 01h44m +50’ 02h20m 02h16m 02h12m +51’ 01h40m 01h36^2„ +50° V552 * • 3 01802 RV V369 Ш142 62 c e 01394 C552-5 ’ 01867 +44° 01612 * 01859 • 01807 Lederman 1 +41° A276 ANDROMEDA 01418 01704 • о M+7-5-27 Ul 303 01332 +46° +48’ +45’ *+41’ +49’ 01796 о 01780 02 20 02h16m 02h12m O2hO8m 02h04m 02h00m 01h56m* 01h52m 01h48m .. - • 909 906 . 41 M+7-6-23 914° Ъ/л\ +42°/1-’^ 911 -.,^Л^7-6-6 °C538-41 .M+7-5-39 01893 . 620 +42° ANDROMEDA • j 66 . I ° M+8-5-5 65,' о _64 © 01830 920 01854 Q M+7-5-43 1827 +43° M+7-6-18 32 #( U1?41 ^7-5-42 • * 01782 ’ 910uL8S8 A347 I ® U1840 ’ &JJ1914 * " ° U18SS +40’ L__ 02h28m 02h24m Г- • 1 • • • ♦. • • • • • • • ♦ • • • • • • • •* ♦ • • • • . • • • • ♦ 650-51 M7 Little Dumb 6 bell • ♦ • • ♦ • • fl 2 • ♦ PE RSEUS ’ • ANDROMEDA * - O1493A ’ , , 01728 01552 U1563 ° PERSEUS- 01634 U1492о .01562 □ • • M+8-4-17 V372 . 0/504 --------—0---- 0 • .01508 Ul 389 60 b V370 • 746 V366 О • 812 O 4 01447 U1355 57 Y • Almach (Almaak) A 3C54 U1331 XZ ’ |.oU 116° ©OP 51 * ( ® V365 01185 01179 ®GY +44° 01162 50 \) L//667 • U1626 . C538-43 BX +40’ 01h44m 01h40m olh36m Nova Quasar Amplitude 2 0 mag 0.0 and bnqntet ^^^^87-200^^.^.- Л|л,|йя | Amplitude I individual member arc P | i.Omag.oil exceeds Amplitude Amplitude 4.0 mag VO may Double or Multiple Stars 6.0 6.5 7.0 7 5 8.0 8 5 9.0 9.5 9.7 if separation Variable Stars Radio Source X-Ray Source
44 +43° +42° SOU 620 о +41° o LM86 U460 ° 19^ ANDROMEDA М4-8-2-12 ®20П 1)475 a +48° J? +49° +50° m oih12m 01h08m 01h04n1 +51° +51° U 761 RV U471 HN® V362 О U665 UZ‘ • - 35 V 0605 ° U522 573 « • U1070 ANDROMEDA• 00h52'n 00h56m 01h00m 01h04m Qlh08m 01b12m 01hl6m 01 h24m 01 h28m ---5— M+7-3-25 1 . U880 • M+7-3-31 477 M+7-3-29 +40° ---- J--------- 01h36m 01h32m +40° 0<Я8» 00b44m 01h36m 01h32m 01h28m 01h24m +52° . . PERSEUS ! • • : •• • ; • • • • ’ RZ^CA! iSIOPEIA. V766 ЗС22 . U576 М+8-2-22 +50° • • M+8-3-29 • • • U10< d> • • • • • • 12 • О Л 0902 • • • ♦ 'l+o-J-IT • ° • • • Q J joj’J • • u> • • • c L 46 . Io 0731 • • _дд— • — —1 1 • 1 • • • 1 +49° •si ®\ OP • 1 . . /365 . U1035 562 о • • э • M+8-3-22 •=» • • • • • • *. • • • • • • i • • I * M+V- +48 1 1 • +47° 1 132 0 • • • • 4 • • 49 • • • • ♦ • *• • • • • • • • • . 42ф ' • . • V < I • • • 1 • • • . CE • • • • • ♦ • 0816^ U813 • • • • M+8-3-11 • • • • • • • о • ♦ * • +46 • ♦ V364 • • • • о • U1068 • ♦ • <48(0 • • • • • • 46C, • • <v A • 3C36 • • • 1 • • • • • • • __ El ’ • +45u +44° • 0 590 • • • • ♦ • • • • • • • о CD • • • • • • 0836 ♦ ♦ • • 1 • ♦ • • • • J I • • IM+7-3-18 ° 1 • 1 —ф— '•41 U826 0728 о OU725 U622 > .7 _ _ >ТЧ U608 • UJ101 17783 • U777 44 U600 U655 39 278 220 Uo.< ____• CASSlOPtlA 01h20m 317A o317B M+7-3-11 +43° V358 ' M+7-3-5 I s’ • M+7-3-6 U539 M+7-3-3 M+7-3-4 •1 +42° EG® Open Star Clusters and Asterisms О 0 to scale < 5’ Globular Star Clusters Planetary Nebulae Ф ф Ф -ф- -ф- -ф- -ф- toscale <$' >30" 30"-10" 10"-5" <5" Bright & Dark Nebulae ° ::: to scale 10’-5' <5' Galaxies 0 I ° ° ° >5' । 5'-2’ 2'-Г <Г to scale 1 major axis Galaxy Cluster '.J to scale 00"44m to 02h28m +52° to +40° AND CAS, PER M Гиюл / Sony Rappoport / Will Remaklus
45 00h04m 00h08m 00h12m 00h40m 00h36m 00h20m 00h32m 00h28m 00h24m U64 ANDROMEDA EC® • V353 +40° U262 4-39° R0 1.1550 ° +38° +37° +36° +34° О U444 Andromeda Galaxy \ 224 М3/ +39’ +40’ 00h44m +41° OOW10 --+41 00h16m 23 SV о CN‘ 24 (J U318 о M+6-1-9 V346 25 6 Andromeda III U128 M+6-1-23 M+6- 9 5 V341 U160 M+6-1-8 29 Л 29 о 3C/9 7836 U232 U284 +33 о ° U384 CR® ©V343 + 32° О U346 U355 U319 © 1/299 C499-40 C500-32 +31° -q- 19 о U117 О 13 20 112 о о М+6-1-16 $ 7S3I м+5-1-31 U334 О* U238 о 226 U433 о М+6-1-26 • о С499-38 1/330 4С+39.01 <3 С500-65 1312904 М+6-1-4 0 I 1.5376 , +34’ +38’ 39О +35’ М+6-1-6 + 370 ____ I +33’ V401 |.5373 ' ^1.5370 -----о------ (34 65 U442 ' О М+5-2-28 . M+6-1-22 0 M+6-1-18 • +36’ (363_________ 1г5 M+6-1-12 • a oV354 M+6-2-1 +30° PS ° M+6-2-14 218. M+6-2-12 • ©V350 oAQ 233 .. о C500-80 U431 M+6-1-30* M+6-1-28 27 p M+6-1-20 +32’ • °U381 315 О U388 о о 149 ^140 M+S-2-23 • * • ° C500-33 ’ о U279 С500-13 о о 1/130 О 43 M+5-2-2 * M+5-2-1 M+5-2-5 OV344 С500-74 О 1.43 t U400 M+.5\2:31 о C500-48 >28 GN +29’ 00h44m ANDROMEDA ----------L 30 Е о ‘ U37L_L_ 00h40m 00h36m 00h32m U310 <У---- 00h28m M+5-2-11 о M+5^2-8 ^97 ° M+5-2-3 > U21S SW LR ’ 00h24m о U166 /q 71 tjo M+5-1-61 74 ol/152 76>72\ о °U147 C4 99-95 M+5-1-63 00h20m 00h16m uw М+5-1 t-55 ъ U93 ьШ02 7819° i PEGASUS’ 1 • M+5-1-27 7806* 7805 U12 +30° +31’ Alpheratz : 21 . 27 -4 00h12m 00h08m 00h04m 1 *+29° oohoom
45 00h00m +41°____! 23h56m 23h52m 23h48m 23h44m 23h40m. 23h36m 23h32m 23h28m Ui2632 23h24m 23h20m 23h16m 2 +41 QQ i oV400 7640 +35° +34° +33° +32° +37° +36° +40° +39° V397 +37 +36° ST • V386 M+6-5/-5 0 V353 73 M+5-55-1 1.5355 SU 64 V348o V356 о 7/99 72 U12864 • 7760 V350 U12476 U M+S-l-4 *M+5-1-3 U12776 ’ О 0 \У\2634 M+5-55-48 о о U12741 +33° +32° +31° M+5-55-30 0 M+5-55-28 0 °U12645 2650 0 . • °U12570 • 7680 .М^55'22 967 ^M+5-55-21 . ' U12693 О о U12666 U12714 M/5-55-45 о /40 +38° OU ® M/6-1-2 /.5370 U12869 M+6-52-3 -V391 U12651.? 14 . M/6-51-4 +30° +29° 00h00m U12861 о v398 * U12672 M/5-55-17 ANDROMEDA U12845 * V360 M+5-56-11 г-.Ц +39° 4 +38° ANDROMEDA PEGASUS U’h +34 C497-7 О О U12538 U12711 , , • ‘’M+5-55-4J Ш2713 Q a Barbon's Galaxy C4 97-42 о M/5-1-8^ . I . о " PEGASUS M+5-56-20 U12803 ' 23h56m 7753 ^7752 v: \ 7729 M+5-55-51 -m+5-55-50 23h52m 79® 23h48m 23h44m 23h40m Open Star Clusters and Asterisms Globular Star Clusters С) о ф © Ф to scale < 5' to scale < 5' Planetary Nebulae V V V > >30 30’-10" 10"-5" <5* Bright a Dark Nebulae to scale 10*-5’ □ P104.2-29.6 0 U12639 о М+5-55-27 ~ 63 23h36m Galaxies lu scale О о 5-Г 2-Г < major axis ‘0 (J12667 О U12657 23h32m +30° U12625 M+5-55-24 M+5-55-12 * M+5-55;9„ M+5-55-7, V349® о M+5-54-56 23h28m Galaxy Cluster i to scale M/5-54-61 М+5М55-10^/о^и12557 ^5-54-60U]2J82 23h16m —Lu/2566-----7--- 23h24m 23h20m 00h44m to 23h16m +41° to +29° AND PEG Zotw) / Barry Rcppufjoa / Wlll Hcrrkji(kli
46 23^24m +41° 23h20m 23hl6m 23h12m 23h08m 23h04m 23h00m 22h56m 22h52m QQ 22h48m 22h44m LACERTA +40° ° 7379 12 DD +41 +39° M+6-50-// 10 +38° L//2737 о SW +37° . о 7395 M+6-50-10 +36° U12236 +34 ♦ о ’ U12156 2/88 3C452 • U12282 o. U12204 о U12199 о . * U о 012181 • 1)12173 М+6-49-70 ’ • 0 DV° М+6-49-76 о sx M+6-50-20 7514 © U12179 ®V345 U12177 7485 О ’ 7449 ? °&7445\ 7446 ~+ ft U12161 U12234 о <7363 7369 • о о О J12206 U12150 о • U12201 U12215 U12157 ° М+6-49-', +33° +32° +31° ® V350 +30° 7640 V381 M+7-4 7-1 AB U72295 М+6-50-18 © о M+6-50-25 M+6-50-21 V386 C497-7 0 012538 64 63 U12372 7440 : О = U12260 •7426 * 22h40m +4 ^V41 'З' V364O © ' М+6-50-7 о -----7 +31 • М+6-49-77 PEGASUS © 012474 V348o 012444 75/2° 012476 V349® 012410 M+5-54-41 о C496-50 °. 0 • 1-1473 o M+5-54-39 4 ®V343 1 0 7490 • • • 1 . 0 ’oV340 1 012323 • 012362 • 012356 * 0 • ' 1 0/2297 J 0 M+5-54-25 : 012385 М+5-54-15 • U12242 М+5-54-8 М+5^.4^О12'235 M+»'54i3'^O12238 ------М+5-54-17 \ °7407 । M4.^.U.7 7 U12252. М+5-54-19 !/ о о М+5-53-17 U12218 • QU М+5-54-12 М+5-54-3 °Ш2149 — +3 .^.U121 , 012311 7473 -° О 7457 54-23 M+5-54-16* 012214. ‘ 012210 i M+5-53-21 O012l85 UY' M+5-54-61 М+5-55-9 о . ; , М+5-55-7 . 012530 М+5-55-10 • ° I +?3 h 24т 12566U,2482 012430 №20т 23-16™ 7420 о • + A2503 23h12m L * •-©------- 23h08^ 23^04^ о 7439 23h00m ’ V339 о 012212 22h56m 22h52m 22h48m Stellar Magnitudes (V) Double or Multiple Stars Variable Stars ® ® © © ® (•) ® ® ® ® © Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag 3.0 mag 4.0 mag <=>7356 oU12164 Matar • • 44 T] о ' 7357 ♦ 012163, 43 0 ___PEGASUS 22h44m +3 22h40m « Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" Copyright C 1987-2001 Willmann-Bdl. 1гк
21hS6m 22h08m 22h12m 22h16m 22h20m 22h24m 22h28m 22h32m 22h36m -7223 Ji 1927 • LACERTA 7282o 12 DD +40° +38° ♦ U12131 M+6-49-36 U12063 . +35° о 7315 М+б-49-i C5 +34° +33° +31 +30’ U12125 . о U12121 7336 U12051 22h04^7i97 22b00m +40° +37’ +39’ U12064 V362- U12073 ° ’ U12075 • M+6-49-48 0 U12137 V418O C514-36 ------—o- OU12060 CX U11862 H11890 C513-10 SY „RZ 29 Л2 U12022 7217 U12071 RV OX о M+5-52-13 HQ 22h00m 22h04m 22h08m • PEGASUS GX +30’ SV RT UH892 uv 72538^ • 0 U11981 22h40m +41’ +36’ M+6-49-67 ' M+7-46-9 M+6-49-15 M+6-49-27.M+6-49-21 U12044 U12016 U12009 . M+6-49-31 OU12006 U12056 U12037 J12040 7273 7274 - 7276 ~ 7250 7248 U11949 • °l U11955 . . U11950 ? О 1.5180 -^7227 • 7228’ U11912 1/11895 +38’ 3C438 7242 . O’ 7240 M+6-48-20 LACERTA • о U1 995 7264 ^ 7263 <£7263 U12007 PEGASUS U11893 _ -7345 .• М+бЪ-бб*073*?" 1 • ^'-M-f-6-49-61 60 1 M+6-49-56 U12127 ’ +32’ ‘S 43 0 °U12039 о U12020 U11975 M+6-49-17 ‘ ° M+6-49-44 7331 ' 4-79 ° 7337 | 231973188,4 • 7343 <7 7 ^oc7\2o Stephan's Quintet • ° Ш 2082 M+5-53-7 U12143 +29° --- 22h40m 22h36m U11974 (JU 994 -M+5-52-4 '•38 • • • 7275 7271 • P7270 9 • • • • • — • • ♦ • • 0 M-vS-53-1 • ®PV * * • • • • ♦ ► ♦ • • 0 °U12011 U12018 • °KX 7292 pp • M+5-52-3 M+5-52-2 ЛЗС441 22h32m 21 7286 22h28m 22h24m 22h20m 22h16m 22h12m ® 4C+31.63 ' C493-15 +29 2^56™ 0 Open Star Clusters and Asterisms О О о to scale < 5' Globular Star Clusters ©Ф Ф to scale < 5’ Planetary Nebulae -0- -ф- -Ф- < >30’ 30"-10' 10’-5’ <5" Bright & Dark Nebulae □ LJ ° •; to scale 10'-5' <5' Ga ^0 >5' to scale laxies О О О S'2 2-V <!’ major axis Galaxy Cluster ; 'j to scale 21h56m to 23h24m +41° to +29° PEG LAC, AND, CYG Wrf hnon / Barry Rappapon I Witt Remaklui
47 LACERTA V2153 +39° +38° +37° +36' +36° 21h24m VW7O® +34° +35° 22h04m 22h00m 21h56m 21h52rn •..*21h48m 21h44m +41 77 21h40m . 21h36m 21h32m 21h28m +40° J — (///895 O1 /4 P86.5-8.8 /2 70 — CYGNUS °V2158 V836 . V460 V2170 +32° +31° C493-/5 •+30‘ +30° CYGNUS PEGASUS 21h24m 21h28m 21h32m 2164401' 7116 21'140rn 22h00m 21h48m 21h56m 21h52m +39° 69 (V2157) «•* .-17063 +37' +29° I— 22h04m +40' +34° +33° U11862 l/J/84/o.« c Ul1890 U1J892 U11893 Q4C+3/.63 3C438 M+6-47-7 ^M+6-47-6 Суд X-2 sV2171 RV • • • • • • • • • Uli 781 0 • • • • .0 1.1392 - U11775 • • • ♦ 5 • • • • • • • • • ’1 г • • • • • • • • • • • » V1073 • • 1 • • 1 • • • □ V2166 C493-8 = VI334 +38° U11 • FT • 743 ♦ • •» • •• - 1 • +291 21h20m A X Amplitude 4.0 map Amplitude 3.0 mag Nova Quasar mdbnnhW Copyr^^^/./OOlWXlmann.BeMnc Amplitude Amplitude 1.0 mag. or less 2.0 mag. Double or Multiple Stars lreJ,v1du4ln»n,bm«pW'd if separation exceeds ьо Variable Stars Radio Source X-Ray Source 6.0 6.5 7.0 7.5 BO 8.5 9.0 9.5 9.7 0.0
58 V ?oh48m 20h44m 20h40m _?V+4V >-20*56" 20h52m 20*48 21h00m +41° +39° V2128 +38° +37’ +35° +34’ m 4 +38° +39’ m 21h08m V2139 & V367 Do 47 66 0 +34 V2021 7037 V2143 +33’ 6974 A 4o +32° DT 6995 +31’ 6960 <>V2150 • UX 20h44m 20h48m 20h52m 20h56m 21 "00™ 21 h04m 21h12m 21h08m 21 h16m +40’ +29 21h20m • . Ru173 V568 +40’ « CYGNUS • • • . 1 • • • • • • • • ♦ $84.2-4.2 ♦ о . ’• • • • . Be 54 • —• — • ♦ ♦ • • VYS 67 a • © • • • • ♦ • • • • • • • ♦ • . • • • Piazzi's Flyinc Star • •• • • .61 (V1803) • о ♦ ♦ * »• • V2145 VI334 <• • -Ф- • • • • • • • • • • • • • 1 • 1 • • ♦ • • ♦ • • • Do 45 1 • ♦ • • ♦ ” • • PK 80-6.1 Egg Nebula ' V2130 +36” VI058 V389^S> " °V2146 V2131 vx • DR Р78.3-2.7 Ru 174 V1056o' >54 к ' +36’ V2137 DoDz 11 VI862 Ru 175 49 +30’ V2142 • • • • • • • • • • • • -<6992 • Veil Nebula 1.1340 6979 ‘ +30’ °7OI3 CYGNUS +29° 20h36m Open Star Clusters and Asterisms 0’0 O to scale < 5' Globular Star Clusters Ф® • to scale < 5' Planetary Nebulae -ф- <- -Ф- + >30’ 30'-10’ 10"-5" <5" Bright & Dark Nebulae <2?<2? ° °::: to scale 10'-5‘ <5‘ Gc > 5 to scale laxies О О о 5-2’ 2'-Г < Г major axis Galaxy Cluster Z’x to scale 20h36m to 22h04m +410 to +29° CYG PEG, LAC, VUL Wtl hnwi / Harry Ruppaport I Witl Remakkn
48 20h44 20h40 20h08 Q? X-3 V2130 CYGNUS DoDz 10 1.1318(a) P75.6+4.3 V455 CMB130 DoS V498 Crescent Nebula 6888 Do 42 6874 Do 40 V2128 V1183 Ru 174 1.4996 6881+3! Be 87 Cedi 74 vdB133 Do 4 7 V441 V382 V1362 Do 1 Hu 173 VI769, B146 6883 VS68 VI749 Ru172 Sh2-101 1.1310 Be 51 P72.1+0.1-6- V2114 Be 84 V485 V2127 V2108 V2111 P7 3.0-2.4 6857 P71.6-2.3 V2113® vdB128 V788 У477 V2123 V2012 V388 P68.8-0.0 Д V442 6894 0- P67.9-0.2 VI027 CYGNUS V2103 20h44 20h40 1.4954/55 ° 20h28 20h24 20h20 20h08 20h04 20h00" 28 b<* (VI624) °V2107 V402 B347 (•- '1318(e) Be 85 Do 41 • 27 b’* •• (V2008) ® 6871 ' ' V453/- ’29 $>(V1644) Wecuu 20h36m • J.DN889 p78.9+0.7-$ 'I ' ) . V405 ) •- • О Do 10 20h04m 20h00 •} -6910 V2118 <*. . ( Do 43 Sh2-108 ’ ’ ’ T V470-- . * • *~P7 7.5+3 7 * * * 8343 1 Do 4 ? J □ bo 3 ‘Sh2-104 V444 •: V 7 P76.4+1.8 Do 37 B145 ___4 _J3e 52_ ‘ j* 20b16m 20b12rn 6913M29" ' / yV2Q31 -P76.3+1.1 4 • . • {'«oV478 <>P68.3-2.7 ' . . ‘ V398 P69.6-3.9 • ’ 3C4IO^V2116 . B144 \ Fish on the Plottt <-r.-:oV448 /" ADS13292 P69.7-0.0 •* • ’ ?\V1768 о» V2099 V2105 c • • Double or Multiple Stars o.o and boghte» 0.S Stellar Magnitudes (V) Variable Stars O' ® ® ® (•) ® ® (•) ® о 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7 5 8.0 8 5 9 0 9.5 9 7 Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 rnag. Amplitude 4.0 mag и Nova Q Quasar A Radio Source X X-Ray Source Individual members arc plotted if separation exceeds 60' 2.0 Copyright € 1987-2001 Willmann-Bell. Inc
4f 19h20m 19h24m 19h28m 19h32m 19h44m 19h56m 19h48m 19h52m ’ V476 +40° + 38° 21 I] P69.2+2.8 © V380 V973 8 Cygnus 4 ’/Vf+7-4 +40° +39° +39° 8144 Fish on the Platter 19hl6n] 20h00m +41° P68.7+3.0 ° * • V2092 о 19h40m 19h36m itJ11460 U11459 6.1 6791 V480 • V2090 I V1125 V977 3C399.1 6834 su HH 19h20m 19h24m 6842 VULPECULA 19h28m 19h32m 19h36m 19h40m 19h44m 19h48m 19h56m 19h52m +30° V1507 • +29° 20h00m V209V • ° ♦ +34 19 (VI509) . • <s>V2093 Skiff /1942.3+3839 U11456 C202-8 * M+6-43-3 + 37°*-^ * V2082 ’ +36° Sh2-l01 • /ygx-z’ VI357‘ 4 +35° Be 49 ° V2097 r +34° V1171 ®V449 +33° -P68.6+1.1-* P68 ^9* 6846 +32° V2099 +31° +30° B341 P69.2+3.8 VI765 SSWZ94 6 P66.9+2.2 V1967 V2086 —11.1303 ----5 ’ 1 1302 UH448 . V2084 V1919 12 0 .* * VI744 ’ X Campbell's < Hydrogen Star V885 Mi 92a ♦ • Footprint Nebula • -o— V556 U11433 •' * • * • _ . • • 1 • ♦ • • • • 21 6 +38° U11426 0 I U11428 V555 +36° 6779 M 56® +29° 19hl6m WH Готол / Barry Rappapon / WtH Remaklus
49 J9h24m mb 10 4 19^20m mb. 6m ^612m 19h()8m i9h^m V476 LYRA +40" +32° +31°* +30° 21 0 +37° +36° 18l®« +36° +35° ь 6692 Uli 399 RY oV555 M+6-41-21 • • ©V535 +34° +33° +32° □ V478 V536 19620m 19h16”i 196l2m 19h00m 18h56m 18h52m Uli 372 ° HM M+6-41-17 о + 30° +31° 1311367 <>P64.9+15.5 .+38° M+6-41-12* 6720 M 57' Ring Nebula 8 V1 __ 19h00m м+лзр-бТЗ M+7-39I . о V547 . • 6745 . ®i ®- . I V543 18h56m 18h52m 18h48m 18h44m 18h40m +41° ©- V541 ° M+7-39-4 4 £’ 6695 • . 0 oV491 6686 U11319Y лпо +40° . 6685 +34° +33° +38° 6791 6202-8 o U11433 *U11426 19 (V471) 20 n V545 . M+7-39-3 St2 0 • V539 •+39° за. Vega 0 1 Ш1428 3C399. / 67™MS6($ . CVCNW \ I LYRA +29° 1 __ _ 19624m Stellar Magnitudes (V) 00 and txigtitf* 0.5 • • • • -.•<1 • 1 • _ • • • • ♦ • 1 • • I • • ° OU • • 6765 4 • •• • • • •- • °RT • • • • • U11380 P68.7+14.8 $V.542 M+6-41-24 12 5i 11 5' 6713 +6-41-20 HK° O 6688 1311325° 1311338 . । U11336 , □ V549 1 14 V Sulafat 15Л о V544 1.1296 10 p 9V2 • • • • ♦ • • • • - 6700 • 0 U11333 9 О EY U11404 »^^ 6743 19 h 08™ 19704т~ — ~ Double or Multiple Stars Variable Stars 18h48m 18h44m Amplitude Amplitude 1.0 mag. or less 2.0 mag. Amplitude 3.0 mag. Amplitude 4.0 mag. +29° 18h40m D Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted it separation exceeds 60" 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright © 1987-2001 Willmann-Bell, Inc.
4S h om 18"04m l8h00m 17h56"10 18h12m 18h08m 18 ° — М+7-37-34 HERCULES 18h24m T ‘ . M+7-37-38*’ TW 2Ц 0 +39° +38° 91 9 V534° V987 +37° U11304 +36 +35° +34° +33° +32° U11219 6686 +40° о Cl 73-21 -9* U11311 О —о T M+5-44 V53°1 +36° +40° +38" +37° 18h40m +41° 18h36m 18h32m 18h28m V530 0 M+5-44-2 94 v V976 M+5-42-29 «UH098 18h00m 18h04m 18h08m 18h12m 18h16m 18h28m 18h36m ®V532 о 6665 M+5-43-19 0 +29° 17h56m LYRA • oV491 LU11^9 6675 • • • • • ♦ 0 • • • • ’ 1.1289 • ^6685 ®XY • .U11313 6663 • • • • • о . • .о 6646 0 1.1288 • • • • • °3«Ш Vega^^ M+6 M+6-4I-6 ^U112^ о ;U11281 41-5 > • • • 78 *' • • • • • °U11312 ’ M+6-4/-/2 • • • Uli 268 V529 •. U11190 M+7-37-33 о ‘M+7-37-36 M+6-40-17 ° I * U11199 о 6612 6657 U11265 6640 »_____ V527- U11303 3C382 . (111275 ' 6662 tUH233 M+5-43-20 +31° . U11291 U11296 * +30° С/72-40 о LYRA HERCULES 18h32m +29° 18h40m M+5-43-16 108 * ' 6585 ° (111140 M+6-39^9 -39-30 W°; 1.1279 M+6-40-6 <9 1111124 M+6-40-7_ Д __ L — — — 1 M+6-40-3! «983 ° о М+6-40-2 о Lil 1087 о • (1111 • • 104® (V669) '| 6575° H'Tl 277 DoDz 9 U11195 U11157 ОИП129 V8150 99 b 18h24m 18h20m 1071 1111076 . Y971 6504 «972® U11058 ♦ ^5-42-41 M+5-42-17 +30° Open Star Clusters and Asterisms ( o to scale < S' Globular Star Clusters фф Ф to scale < 5' Planetary Nebulae >30” 30"-10M 10’-5" <5H Bright & Dark Nebulae <2?<‘°° to scale 10'-S' <5‘ Ga >5' to scale laxies О О О 5'2' 2'-Г <Г major axis Galaxy Cluster ( 'i to scale 17h56m to 19h24m +41° to +29° LYR HER, CYG Wd T'mon I Barry Bappaport / WW Remaklus
50 Variable Stars Double or Multiple Stars ! Stellar Magnitudes (V) Q A X Nova Quasar Radio Source X-Ray Source Amplitude 2 0 mag 5.5 40 45 50 00 0 5 10 and bciqhte 6.0 6.5 7.0 7.5 80 8.5 90 9 5 9.7 plotted Amp”k^ss %- I 1 0 mag or less Individual members are | it separation exceeds 60 Copr.gh(C «987-2001 WHImonn Bdf. inc
5 horn 16*48" 16*44" 16*40" 17h20" 17*16" 17*12'J 17*08" 17*04" 17*00" — +41’ Г-Ш0812—।--------о---- Я)6339 М+7-35-50 6-2 ’ М+7-35-62 М+7-3 М+7-35-61 6320 +40° V947 о +39’ • М+6-3 +38’ 69 е +37° +36° +35’ + 34’ 6349 M+6-38-18 о 16*36" _— , +41 V939o M+7-35-35 М+7-35-11 М+7-35-9 , 0 М+7-35-12^ i ? ! Л° М+7-35-18 М+7-35-19 о М+7-35-33 м+7-35-20 М+7-35-38 ® о| V937 М+7-35-42 ' М+7-35-52 о 8-12 1.1245 °Ш0785 67 Я gUW 1.1249 9 М+6-38-4 <5 M+6-: 8-5 С198-32 68 и ® 72 w 0 . U10801 +33’ +32’ ♦ <? С170-10 +31’ +30’ HERCULES +29“ ’ 17*20" OV929 М+7-35-13, о . U10599 О 6257 * М+7-35-7 U10553 HERCULES V .М+7-34-125 о M+7-3J-138 М+7-34-13^ М+7-34-143 +40’ 3C345 м+7-34-133 Л?, М+7-34-132 62 2 ‘М+7-34-136 М+7-34-139 оМ+7-34-130 М+7-34-131 +39’ М+7-35-26 М+7-35-15 V932 DoDz 6 U10635 О 6255 М+6-37-18 о U10677 с М+5-40-47 M+6-37-19 о U10706 U10732 1.1244 . ° М+6-37-29 о U10708 <• М+6-38-1 М+6-37-23 44 П U10547 V911 U10529 Х/910» 58 е U10668 U10673 * С169-12 ° М+5-40-25 16*40" 16*44" 16*48" 16*52" о 6282 010663 и 10662 +30’ U10679 U10675 RV М+5-40-43 о U10712 . U10715 6274 V359 М+6-37-20 ®61 (V931) о U10688 1 • ♦ :ч ;» A2249 • M+6-37-32 * M+6-37-31 • • • • ♦ • • • • • • • >59 d • - • • U10733 • 1 • • / 1 • 1 О U107490 о 6330 70-5 17*16" 17*12" Her Х-1 M+5-40-21 V914 о V912 +38° UU Open Star Clusters and Asterisms to scale < S' U10567 ЪШ0566 М+6-37-11 С169-7 V923 М+6-37-2 М+6-37-1' 6207 о 1.4617® Great OU10OT 14614 о 6194 6196 9 _ +36° 6197^ V902 М+6-37-4 0 о м+5-40-38 U10714 V9°38 * 17h08m Globular Star Clusters to scale < 5' 50 48 17*04" Planetary Nebulae >30" 30"-10’ 10"-5" < 5" 17*00" V645 __® _ 16*56" Bright & Dark Nebulae to scale 1 O' - 5' < 5' Galaxies >5 5-2‘ 2-r <r to scale I major axis Galaxy Cluster to scale +29’ 16*36" 16h36m to 18h04n' +41° to +29° HER Wit Tirnn / Burry Boppaport / VWH Remakkx
51 1б^44т +41°,__^26\0m 16^ А2197 | м+7-34-1з8 /ЗС345~^ М+2'^143 ^м+У-з^зЗ I о М+7-34-136 • М+7-34-139 -1 ^+2-34-131 +39° I _ I • M+7-34-125 У1Р512 ° * ™ 7 — ^+7-34-136 • ^M+7-34-130 6195‘ 16^ 16^28^ Л, 4* 010459 m+7-34-90~6!74 6,^2. М+7-34^23»<’м^34-82,81»6Н66Ч47° 6141o , 6180 14+7-34-33^ ^M+7-34-27 o' M+7-34-47.°l 2" I U10357 ♦ ' v J-^+7-34-28 ' _ M+7-34-62,61 16hl6m 16h12m »16h08m 16h04m 16h00m -H------------1 +41’ М+^-^г^^мТГ-зТУГ^'— --1_______ ^u,0349 u,033° M+7.34.0S^O ^.010404 ^^^41 M+7-34-104 U'°420 6166 M+7-34-19^ 3- --1--362 • ' M4-7.34.79 ^М^7-34-26 ... Г... М+7-34-67 о L 6158 J ° M+?-^334 18 ° М+--34-'0 М^7- ^М+7-34.^Ы^З^ "CN ' ^34-37 ПМ+7'34-^ I ’I'' ’ • М^34-5613' 1.4610 P61.9+41.3 44 q +38° - ' . •iUy iuu •) C196-50 DoDz 5 '• HERCULES 6058 U10166 U10155 +40° ° 6069 +39° +37° +36° i У 1630+377 ! M+6-37-21 , OUI0477’W о J ^~~~~~Jm+6-37-i I ^+6-36-50 0 6207 I ----4-•—_____I ГТйЗйгй** I ’ I <17 Г 0 010473 • \б1№°*!94 ’; • ° V896 ' М+6-36-42 о i 25 ° U10344 ci • M+6-36-IX . ^м+б-зб57Г^т/ 6'37. 6122O,S'*V Al 6120 ’ M+6J6-5 . о M+6-36-9 ° w ° и 10257 +38° 6142 О М+6-36-24 & 6117 ®- М+6-35-46 о М+6-36-3 о M+6-36-8 М+6-35-41 о ° 6038 М+6-35-34 М+6-35-24 +37° 6126O U10342 О M+6-36-4 16 Т OU10227. М+6-36-34 о M+6-35-36 о М+6-35-25 М+6-36-43 М+6-36-40 О м+6-36-31 м+6-36-33 ♦ М+6-36-6 АН +30° +34° < +29° I6h44m 6097 9 о 6109 6107 6Ю5 M^-6-36-12' • M+6-36-23 • I’ о M+6-36-20 • 6116'6114 . I О 6185 ' <§> • 6179 9 М+6-35-40 6103 • М+5-38-52 U10312 RY М+5-38-39 ‘ о U10372 'А2175 HERCULES j CORONA BOREALIS I6h4oni 18 U £> 20 V' *21 VJ M+6-36-53 . V899 ----I.___U10445 • Cl67-559'" \. ' U10262]o \ U 0259 ’ ; 6086 о \ 6085 0 M+6-37-4 01 U10504 +31° M+6-36. 6177 ♦31 Ф-17О TZ "SX 6163 ч6,162 7 6h28m BE. I6h24m 6089 3C332 16h20m I6h16m 16h12m Stellar Magnitudes (V) Double or Multiple Stars о M+6-35-44 M+6-35-29 M+6-35-31 15P M+6-35-27 • о M+6-35-32 0 .AD +36° +35° + 34’ +33° М+5-38-12 +32° ° U10207 ,AF /А2162 / • AC o U10234 +31’ ° АС о U10205 +30° 16h08m 16h04m +29° 16h00m Variable Stars • Ф ® (g) ® ® (§) © ® @ © 0 Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. Д Nova Q Quasar Д Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60' 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright © 1987-2001 Willmann-Bell, Inc
51 I ©52 V1 BOOTES • HERCULES о 5950 M+7-32-44 12k M+6-34-14 • о -26 M+6-34-22 M+6-34-28^ SY 9 Л U9910o M+6-34-23 0 6013 +40° +39° 0 M+6-34-27 15h20m 15^16^0 M+7-31-53 _________I о M+6-3z € 5966 U9834 oYY XYo M+6-34-24 Xo A2124 11 К M+6-35-1 XZ Э 49 6 M+6-35-8 ' M+6-35-5 1.4539 BU 1)9809 BOOTES ° C167-1 C165-54 48 X 1Sh20m i5h24m 15h32m 15h36m 15h40m 15h44m 15h48m M+5-37-23 0 U10034 *------ о М+6-35-7 Ц +30° ° UU • 0$ 5924 ,h4,m 15h32m 15h28m 15h24 16h00m 15h56m 15h52m 15h48m 15h44m 15 40m 15 ______— +41° fr——1---------г----------------[~ +40° +39° +38° +37° +36° +35° +34° 15 p +33° +32° +31° +30° 141 M+7-33-19 ____Q____ •01/19122 CORONA BOREALIS • <5 M+7-33-5 0 U10065 RS ° M+6-35-18 U10120 —Q____ о M+6-35-11 M+6-35-15 M+6-35-12^ ZZo U10104 G___ Z« +29° L 16h00m 15h56m SWo RRq • 15h52m 54 ф M+6-34-25 . M+7-32-14 M+7-31-52 6Ц 0 U9922 M+6-34-15 М+б-34-lo о 5974 о Cl 66-23 51 U’ ф Alkalurops 3C32O& : • fM+6-34-13 О M+6-34-16 ' A2092 1.4549 5961 M+6-34-10 BOOTES M+6-34-1 < • 0 0 M+6-34-2 +3go 1.4542 о A2067' 2П +36° +34° ‘ M+6-34-5 A2061 U9831 +29° I5h16m Open Star Clusters and Asterisms (} C> 0 to scale < 5' Globular Star Clusters ф ф Ф to scale < 5’ Planetary Nebulae -ф- <> -Ф- -6 >30’ 30"-10’ 10--5’ <5" Bright & Dark Nebulae ° - to scale 10 -5' <5' Ge 2^0 >5’ to scale laxies 0 0 0 5 2 2-Г <Г major axis Galaxy Cluster •' \ to scale 15h16m to 16h44m +410 to +29° CRB HER, BOO Wrf Tirion / Barty Rappoport / Wilt Remokhn
52 l5h20m 15hl 2m 15h08m 15h04m 14h56m 14h52m +40° +39° +38° +36° +34° +30° m m 51 5732 15^24^ 4-41° 4 +39 <? 09473 15h00m ^+7^T-1^ 15h16m M+7-31-28 5853 09623 1.4500 M+6-33-5 ° RY 09537 5727 1-4542 J 1.4496 1-4539 °UU о U 5924 09809 42061 2 J] M+5-35-11 ° 09588 09831 1 0 rr 48 7 l5h20™ 7 5h7 6m BOOTES 15h12m 15h08m 15h04m 15h00m 14h48m 14h44m о U9504 о 1.4505 0 M+6-32-87 . 5789 о 5773 5771 °0 U9519 о О 14h56m 5780 1 4h52m M+7-31-39 М+7-ЗГ^М+7-31- M2 +37° 42067 '' 4-29° 15^24m BOOTES M+7-31-S3 M+7-31-52 M+6-34-1 M+6-34-2 М+5-36-10 Stellar Magnitudes (V) 09691 c> | 42 p ф Nekkar ° 09716 M+6-33-20 o M+6-33-19 M+6-33-22 M+6-33-17 U9647 ° M+6-33-9 Cl 65-13 Double or Multiple Stars • 0 • M+7-31-7 (d S772 • <s> 1444+407 • • • о •• • • • ORR • • — * M+7-30-65 r7rS.5753 5755 S 5752 5754 1.4515 1.4520 . M+6-32-89 ER o* U9560 U9562 09518° ® • U9510 Variable Stars @ ® (•) ® ® (S) ® о Amplitude Amplitude 1.0 mag. or less 2.0 mag. Amplitude 3.0 mag. Amplitude 4.0 mag 0m +4 +4C +38 +37 о M+6-32-M . ° M+6-32-85 +36 + 35 +34 +33' +32' RW +31 +30 •J +29' 14h40m u Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted it separation exceeds 60’ «d^tet 0.5 1.0 1 5 2.0 2.5 3.0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5.9.7 Copyright 1987-2001 Willmann-Bell, Iik
52 +41 <+» .ццт 14h00m »46”- к 14М6» 141'08" 14h4Qm 14h36m 14h32m 14h28m 14*24™ ____ __ — — о +40° —0 U9441 • ° U9386 5708 • 0 U9379 • U9429 * ° М+7-3 0-28 ° М+7-30-35 4 • Ь U9376 ♦ М+7-30- 34 • М+7-80-23 +37° +38° +39° • • 5698 о М+6-32-80 » ° • М+6-32-79 Seginus 27 у U9291 °V 1.4446 ° СР ^87 . Z Л ,4 ъ М+6-32-74 М+6-32-82 * 5695 г> М+6-32-78 о. U9320 & 0 М+6-32-63 F5684 5686 5675 о . о 5654 U9350 . +36° +35° © BW U9372 М+6-32-56 ♦ ’ о М+6-32-54 М+6-32-68 о М+6-32-70 „ М+6-32-47 \ U9315 .*5646 5656 М+6-32-69 о М+6-32-64 М+6-32-66 М+6-32-76 М+6-32-58А М+6-32-57 +33° +32° +31 +34^ 5727 о 5653 1.4447 о 1.4460 о М+6-32-51 о М+6-32-52 5™6 о U9425 5709 5672 +30° 5685 ф 28 6 BOOTES +29° --- 14h40m 14h36m с 1.990 5625 U9242 о 1.4435 -29-27 15371 о • M+7-30-5 1.4394 о 5541 *0 5536 +40° +39° ,09216 ’ 5603 . 5601 5598 0 М+7-29-62 ° М+7-304 1/922? ~^9203| 0 5582 М+7-30-12 М+6-32-17 СУ U8945 о 5596 о 5401 5616О о U9262 —о— U9213 M+6-31-82 +36° М+6-31-77=> о5499 и9042 5517О 5399 Ц31Ч М+6-31-29 о М+6-32-31 BOOTES U9081 о М+6-32-40 о М+6-32-48 М+6-32-39 25 Р 56~39 п 5642 5515 о 5497 U9088 1.4380 U8917 U8960 . 5407 М+7-29-41Ж °* __10— U8962-* ' US’80 54С06 М+7-29-37 о 08923 0 U8975 М+6-31-42 ^5403 М+6-31 -4 3 М+6-31-44 14h32m 0 5657 5545 • * 5557 <=> 5544 • М+6-31-86 ° ° 5524 5529^ 5527 5572 ° м+6.3р87 М+6-31-62 о • U8984 U9022 ^^+5-31-66 U9003 5378 .о 5394 5з80 5^95 U8854 RW U8858 +38° М+6-31-37 М+6-31-74 М+6-3 -36J О М+6-32-24 о DR 0 5623 5611 U9241 09253 о U9045 М+6-32-9 О о М+6-32-8 ‘ +34° U9284 О < U9113 5533 £5568___ I 4=5609 5614 о и9221 U9243 5444 5421 1.4370 1.4357 U9012 5512 1.1012 1.4422 С163-14 М+5-33-41 CANES venАТЮ ®С1 14h00m 14h04m 14h08m 14h12m 14h16m 14h20m 14h24m 5375 0 0 1.4409 U9035 М+5-33-48 о М+5-33-47 1/8999°, +29° 13h56m 5433 . 1 А I пг ® М+6-31-92 „ М+6-31-95 5589 I ° 5590о0’о „5567 . 5579 ' 1421+330® с (J9214 1.4403 14h28m о М+6-ЗГ84 U9107 М+5-34-3 U9048 I i44l“ ЗС294 • о М+6-31’70 М+6-31-65 1.437 М+6-31-49 \ U8856 +30° С162-29 Open Star Clusters and Asterisms OO o to scale < S' Globular Star Clusters ® ® Ф to scale < 5' Planetary Nebulae •<><>•+ + >30" 30"-10" 10"-5" <5" Bright & Dark Nebulae n ^-1 D ::: to scale IQ’ S <5' Ga >5' to scale laxies О О о 5'2' 2 Г <V major axis Galaxy Cluster to scale 13h56m to 15h24m +41° to +29° BOO CVN,CRB
53 +36 BO +40° M+7-29-27 U8917 14h00m 5410^^' 14h04m +41° M+7-29-4 L U*960 ;J4O7 5406 M+7-29-37 usm M+6-31-42 5403 +38° .«CY M+6-31-43 5394 U8945 +37° ° 5401 U9022 M+6-31-37 0 U8984 5444 o 5421 5399 о M+6-31-35 0 M+6-31-29 M+6-31-44 5’ 5445 • r 1 ^S440 5441 ° . M+6-31-47 13h56m 13h52m o -0 5355 5350 s"! U8841o ”‘ M+7-29-14 \°U8851 5378 1 3h48m 1 3h44m , M+7-28-78 5353 5^4 M+7-29-2 5*1 5зРЗТ^^ 0 le 0 1.4336 .° CV о л ! + 5326 1 • U8736! 5346 о 1)8742 9 U8726 13h40m 13h36m 13h32m 13h28m 13h24m 13h20m +41' 1)8670 bi)8651 M+7-28-47 M+7-28-32 M+7-28-35 M+7-28-23 CANES VENATICI 5093 о 23 9 +40’ 5361 Q. 1)8793 -. I5?5 । 5303 о U8683 ° U8621 CM +39° u 5395 RW о 5380 M+6-31-18 M+6-31-17 b U8854 • 5351Ъ 53495341 ° 1.4341 8^ 1.4340 U8760 • . 5305 M+6-30-89 o r~y--------- M+6-30-104 5352 о 1)8833 M+6-3 1-36 О A1813 U8754 0 M+6-30-94 M+6-3 0-91 o°U8739 AW •5267^ M+7-28-48 A 3C288 о U8619 * о 5243 M+7-28-15 U8471 о о U8564 . U8554 о M+7-28-21 ®BM • о 5112 * о . 5107 +38’ VY M+6-30-73 M+6-30-70 ----£___ 0 M+6-30-71 • . о 1,4269 о M+6-30-32 ©CL feH +37’ RY M+6-30-79 о M+6-30-80 . U8693 o 5265 25 QCP ° M+6-30-38 . M+6-30-42 * M+6-30-18 C190-4 . 5,43/l 5142 - 5141 . M+6-29-80 £5273 5276 cs M+6-30-65 n_________i— M+6-30-57 1)8600 ъ 5240 о M+6-30-41 U8583 $5228 о 0 5223 5233 5154 —Cs--- 0 5149 M+6-30-21----- o5/99 oM+6-30-26 * • ьМ+6-30-17 - о +36° M+6-29-83 M+6-29-82 О M+6-30-9 +35’ M+6-31-38 M+6-31-65 >Al 793 +32° CU® +31° +30° ?M+6-30-106 5319 5318% * .5321 CW +33’ U8718 ’ ^M+6-30-84 cp U871T U8715 +34° 14h04m 14h00m 13h56m 13h52m 13h48m 3C293 М+5-33-18 л| 0 U8824 t 1.4370 1.4371 5433 . M+6-31-31 о о • M+6-31-49 1)8825° o 5347 • M+6^31-15 ~^~U8829 M+6-31-25 * 1.4357 M+5-33-39 M+5-3 3-41 M+6-30-45 ________• M+6-30-13 '8S3O +34’ . U8856 4 Cl 62-29 A178V™ Stellar Magnitudes (V) М+6-30-67 Is M+6-30-66 U8609 1.4305^ 1.4304 1)8561 0 M+6-30-49 о 1.4302 » M+6-30-27 M+6-30-7 C161-103 U8685 о 5282 5q71 P—5277 - a 5274 5275 13h44m U8630 о M+6-3 О • 1)8627 • M+6-30-64 1)8605 о M+5-32-50 о M+5-32-49 5259 13h40m Double or Multiple Stars ... „ , .s ... » = ... • • “ “ » ” u “ ° ” ” - and bughtei 0-Э ------------------------------------- Individual members are plotted И separation exceeds 60" M+6-30-34 ‘ /М+6-30-35 0-44* U8539 M+6-30-31 M+6-30-29 . M+6-30-30 • 5166 08431 о 08451 c 5157 U8S6° o’o8548 M+5-3 U8498 0 о U8492 2-35 ^U8496 U8502 о < ----5187— s 3C286 • U8466 U8483 O U8510 13h36m 13h32m Variable Stars о M+5-32-17 13h28m M+6-29-81 • ° 0 50988 о -----5096- M+6-29-84 M+6-30-3 M+6-29- 5098A +33° ^27 • м+5-32-1 M+5-32-4 ° 08397 0° r - 08399 %’392 — ------------Г"* 5131 1321+294s 13h24m +32’ +31° Q161-19 +30’ COMA BERENIC —1 +29’ 13h20m Amplitude Amplitude Ampl.lude Amplitude 1 0 maq or less 2.0 maq. 3.0 mag. 4.0 mag. я Nova Q Quasar A Radio Source X X-Ray Source Copyright C> 1987-2001 Willmann-Bell, Inc.
53 13h20m +41° --- 13h16m 13h12m 13h08m 19 23 +40° +39° +38° +37° 20 AO °5093 ° 5083 • 18 ru M+7-27-45 . In 0 e A1691 < • 16 * 17И15 М+7-27-49 о о M+6-29-75 M+6-29-67 SOOS . +36° 5033 U8303 о M+6-29-72 5002 . о ° SOI4 U8338 +35° U8323 a М+6-29-66 о U8318 0 о RS 1.4201 1.4213 4986 о M+6-29-46 M+6-29-S6 +34° M+6-29-70 M+6-29-73 * о BL % U8266 • U8246 • M+6-29-59 „ ° ______ «>М+6-29-58 M+6-29-63* U8299 5098B < +33° S098A 5096 U82S0 о Q 1308+326 +32° Cl 60-172 +31° ^S074 °- 5056- о C160-190 0 °C16O-17S +30° +29° 13h20m 12h40m +41 12h48m 12h56m 13h00m 13h04m 1/7774 12a e Cor Caroli 4916 1.4182 о 4868 о 1.3904 Q 4861 4959 1.4166 —tf— U8179 1.3892 & 1.3895 1.3810 о о M+6-28-42 4846 о о M+6-29-1 о M+6-29-28 <2 M+6-29-37 M+6-29-43 Q ’• 1248+401 о M+6-29-21 1.3850 U8199 4lS6 О о 4914" , 1.4112 4893 .4870 01.3967 о 4687 U8207 1.4188 в 1.4187 о ° _ U8203 u8181 +40° +38° +39° 4736 M 94 12h52T • oCC IS 1257+346 M+6-29-11 M+6-29-15 • 1.4189 -------0----- ’o «14 1.4199 1.4086 о * .a 1-4049 U8139O о 1.4028 oI.4108 1.4123^1.4118 1.4103 M+5-31-67 ~НМ°зТ42 12h44m 10» U7816 4619 U7811 1/7836 U8076 12h40m 12h44m D.... U8004 1.826 •+34° ; +32° +30° oo C160-30 M+5-31-22 +33° +36° +31° U7812 М+5-31-127 М+^49°262 ^ 4949i4Q88^8fjj42 U8025 о •ч Д1656 M.S-3MS | ° .JJ8069 12h56m <•> 1.4060 1.4100 О s. • 1C280.1 1.4165 ‘ 9 • 1.4064 0 1.4065 °° I- • • • 40S6 • • • Oo 1.3975 1.4003 o 1.3726 1.3783 q1246+377 1.3816 4774 4655 1.3687 0 4662 * U7949 TX. M+7-26-32 0 о M+6-29-6 1.3966 M+6-29-10 M+6-28-44 . 4711 • о 4737 • U7916 4719 o M+6-28-22 4627 =2=4631 M+5-30-115 0 M+6-28-12 U7799 4583 • 5025 ’ M+5-31-151 0 о M+5-31-147 CANES VENATIO ш.5-30-64 COMA BERENICES о U8294 1/7978 O5041 M+5-31-158 4676A Mice ’ 46768 0 o M+5-30-74 M+5-31-167 O 5089 >U8377 J • • * 0 052 • • C160-151 1.821 ° 1.818 13hl 6m Open Star Clusters and Asterisms to scale 5004 8 5004A 13hl 2m M+5-30-87'i <s> 1304+29SJ M+S-31-139^ j 4966 0. 13h08m 13h04m Globular Star Clusters Planetary Nebulae to scale < S' >30" 30’10" 10"-5" <5" 13h00m 12hS2m 12h48m Bright & Dark Nebulae to scale □ >5 to scale Galaxies Galaxy Cluster ID’S’ <5' S' 2 2 Г < major axis to scale +29° 12h36m 12h36m to 14"04m +41° to +29° CVN COM, BOO Wit Tmon I Barry Rappaport / Witl Remaklui
54 8 ₽ • Chara 12h36" 12h32ni 12h28"i 12h24m 12h20m 12h16m I2h12m 12h08m 12h04m 2 +40° M+7-26-7 ° M+7-25-21 —4145---1 10 ° 07175 +39° <•> 6 U7098 U7208 о U7159 1.3014 1.3022 • +38° U7207 4190 +36° +34° +33° о U7071 M+7-25-15 0 U7213 12^44т +41° M+7-25-61 -4_____ ____ Ibu - ° UW(> 07125 M+6-27-20 ° I 0 07105 ° ^M+6-27-16 M+6-2 7-17 M+7-25-13 C215-17 • * 4156^ 4151 l2h40m ( 4655 ° 1-3726 URSA’MAJOR • 07774 07678 07719 • U7816 4534 4619 1.3001 U7007 1.3002 +32° 0781Г 07428 1208+322 076980 1.3330 M+5-29-66 07673 0 4414 о U7750 4514 o U7131 о 4136 4525 <3 o. 1.2992 о M+5-30-9 U7084 о U7H2 о 04148 U7187 1218+304 4308 о ° 0 • 4150 M+5-29-12 * ° 07064 • & O7085A О 4314 - 4062 3C270.14C <SL 07388 4229 I 4227 M+6-27-25 r,M+6-27-22 U7243 M+6-27-33 , 1.3687 '0 M+7-26-28 i M+7-26-24 I +31 4631 4657 4656 M+7-26-23 U76^ M+7-26-30 Q U7699 12h00m — +41 4662 +37° Up 1 AX M+6-28-6 4627 М+6-28-22 о 4-29° 12^44^ M+6-28-12 I M+6-28-11 07799 4583 U7812 M+5-30 Z '4509 M+7-26-5 M+6-27-54 U7599 о 07559° U7605 07598 +30° M,^-30-64 07836 12h40m 12h36m 12*32™ .... CANES VENATICI COMA BERENICES Stellar Magnitudes (V) ° 4495 4395 12h28" CANES VENAT Cl C215-50 • •+40 • • • 4244^ • • о U7145 4214 4163° — U7257 + 39c +38c M+6-27-46 М+6-27-50 M+6-27-48 4359 07395 0 0 • Mi-6-27-32 ----a______ M+6-27-34 o M+6-27-28 M * U7212 M+6-27-41 « M+6-27-31 -4203 12*24™ andbnghkr 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8 0 8.5 9.0 9.5 9.7 M+6-27-8 - -—о--------- о 4097 о М+6-27-2 +37' +36 +35' •.+34' CJ 41 ° 1.30 22 03 • • • • 4031 Cj U6997 3C268.2 +33! +32' M+5-28-74 +31 о 1.2986 4286O 0 4283 4310 4278 о 4272 . • 1215+303 Q ___ ♦ ГГ779~ *4253 4274 O424S 07017 ^0 (j/012 eHY +30 12h20m 12h16m ТЬ о ^1^3 The Box , 4j69 4175^\ 07190 ^4П£_1^_,__4134 2 12h12m o- M+5-29-24 №4131 &4132 12h08m M+5-29-3 --------d Double or Multiple Stars Variable Stars Amplitude Amplitude Amplitude Amplitude 1 0 mag or less 2.0 mag 3.0 mag. 4 0 mag ° 07031 12h04m — +29 12h00m и Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60’ CnpynrjhrO 1987-2001 Willmann-Bell, Inc
11h28™ 11h32™ ц*20™ 12h00™ +41’ --- 11h56™ 1lh52™ 11M8™ 11M4™ 11 MO™ 11h36™ +40° +39° +38° URSA MAJOR U6531 06529 ^ 06817 ' 0 M+7-24-32 06497 о RU S4C+38.31 3930 M+6-26-38 Cl86-30 - M+6-26-13 3941 4025 0 06792 06955 О о M+7-24-17 о М+6-26-56 М+7-25-7 О I > 06916 М+7-25-13 М+7-25-5 U6893 0 M+6-26-50 ® । Groombridge 1830 +37° ® <. M+6-26-44 1.2950 M+6-26-15 11^24™ 57 1.2861 M+7-24-25 e> I M+ 7-24 -24 о M+7-23-40 06433 CX® M+7-24-6 3648 M+7-24-1 ° • o' M+7-23-41 06454 06551 06517 -а1275 06455 3665 0 3658 0 3652 +41 +39° +40° +36° +35° +34° +33° +32° +31° +30° о О 06929 06945 о • M+6-26-67 $ M+6-26-66 M+6-26-65 • • ♦ о C’l.2973 06892 ^3991 3994 о9 1.2979x2— • 3986 „1.2986 о 1-2985 06716 ----- TV® 3813 06639 0 M+6-26-22 0 M+6-26-18 о 06827 M+6-26-16 о 0 3966 3755^ M+6-25-74 (186-63 ---£2--- 3897 M+6-26-35 . 61 06603 06499 о M+6-25-79A 0 • ]695 I ; 3700 о 06570 06526 0 3694 M+6-25-71 I° M+6-25-70 3935 ° о 06900 4020 1 О - 06927 о 06987 3971 06777 о о /.2967 -HS 0 06491 О 1.2928 •_ °U6S12 М+6-25-72 д|257_ J U6397 M+6-25-59,'<0 06393 й о 06338 о M+6-25-42 А1228 1.2744 1\ бо 1.2738} о М+6-25-43 55 • U6307 • _ 06326 +38° HN +37° t/6298 (J6303 о . о M+6-25-32 +34° +W 4С+29.45 ^3984 • q 06853 +29° — 12h00™ 11*56™ 11*52™ M+6-25-62 M+6-26-120 Alula Borealis M+6-25-73 U6337 .o A1336 .• М+5-27-86 1.2947 -Л 128+315 3891 М+6-26-3 о M+6-26-5 о 06659 M+6-26-10 '06610 M+6-26-26 0 I A 3(265 о 1.2957 --M+6-25-51 M+6-25-50 3847 .2953 3855 3878 ' 3880s 3881"° 3871 М+5-28-32 О М+6-25-61 М+6-25-68 - A1213 06761 11*20™ 11*24™ —©- -- +30° 3788 3786 < 3793 62 06545 ое» М+6-25-63 М+6-25-65 -НО 0 C156-84 06367 о д U6355 1 Al 365 06664 3C261 ли AW о 3687 11*48™ 11*44™ 11 MO™ 11*36™ 11*32™ 11*28™ M+6-25-37 <5 M+6-25-36 Alula Australis M+5-27-49 e 06314 +31° 06292 ° • к URSA MAJOR j- +29° ЦМ6™ Open Star Clusters and Asterisms to scale < 5’ Globular Star Clusters ф ® ® to scale < 5’ Planetary Nebulae 4». >30' 30"-10" 10"-5" <5* Bright & Dark Nebulae <?<J □ □ ° =--: to scale 10' 5' <5' Ge Io icale ilaxies О О о S'2' 2 Г <1 ITld|Or dXIS Galaxy Cluster ( 4j to scale 1V16m to 12h44m +41° to +29° UMA CVN, COM и-W ГГгюг»/ Buirykoppuport/ Will RemokkiS
10h56m О 3468 11*24™ +41° --- 11 h20m 11*16™ 11 *12m ° M+7-23-40 +40° 3648 ’ +39° 3658 i f^+724:1 О М+7-23-41 55 06307 о +38° +37° +36° 3C254 M+7-23-36 11h08m ' Al 187 ^М+7-23-29 0 3652 ®сх 10*40™ о М+6-25-59О 06393 * +34° -- М+6-25-6/ < +33° I +32° 131° +30° URSA MAJOR +29° I----------- 11h24m 11h20m Hh04m Л М+7-23-19 Moyall's Object * 11h00m 49 06?2/ о (.2616 ° 1.2617 о 1.2620 М+7-23-8 о 10h44m 10h48m 10h52m 47 (75 996 ° 1/5838 M+7-22-60 LEO MINOR m+7.22-61 +40° М+7-22-46 * О М+7-22-44 о (75839 URSA MAJOR М+7-22-58 М+7-22-43 М+7-22-57.Л м+7-22-52 х ? М+7-22 I 1 q ___—— +39 о М+7-22-76 05819 05804 1 • л-51. М+7-23-2 к J6*j32 ----М+6-24-47 + ~ O (76089 М+6-24-20 0 М+7-22-69 М+7-22-54 1.2607° ._____L ---------—I , 1.2606 :: М+6-24-30 +38° U6326 U5806 o 06002 ! М+6-24-32 ^М+6-25-6 М+6-25-29 . М+6-25-3/ М+6-25-9 3540 Lalande 21185 о М+6-25-1 М+6-25-3 © CO 0 05868 > | О М+6-24-13 М+6-25-25 о о» М+6-24-39 о М+6-25-42 С/55-78 3569 с М+6-25-18 -М+6-25-5/ М+6-25-50 Q 06276 U6036 • i 3432 ° 1)6274 о М+6-24-42 (76338 1/6303 Uo291 • О 3334 О .° М+6-24-7 @ М+6-24-38 (76273 » , 0 0 о W279 М+6-25-32 (76397 /.2744 47228 <£ 7.27381 7.2757 ; '>? U6394 ' 0 М+6-25-43 М+6-24-44 ♦ M+6-25-5 . "W83 OU6 43- +34' 46 (76070 М+5-26-37 М+5-26-7 о 1/5984 U6271 43 • (76031 U6220 3486 10*44™ 10h48m 10*52™ 10h56m 11h04' 11*00™ 11*08™ 11 h16m 11h12™ 05885 о М+5-27-49 о 063/4 о М+5-26-2 о U6198* VX о О М+5-26-51 М+6-25-37 <5 О М+6-25-36 М+5-26-46 : о , —. Д/2/3 06292 о \ +30’ +35’ Оно 54 V • 1/6337 , ’//гэг? Alula Australis U6j67о о 06355 LEO MINOR +29„ 10h40m о (75936 U5813 +36° М+6-25-21 М+б-25-15 - 3545ДВ, с М+6-25-14 --------J------— 3542 О М+6-25-22 д ^252 М+6-25-12 о о С156-27 (75983 U5870 338/ о oUY М+6-25-8 М+5-27-5 —•—а О (76152 vw М+5-26-47 : 05990 о 46 . oUV (75829 : о M+6-24J4_. 3442 • о U5898 о М+6-24-22 3396 3395 3424 о 2 3413 I. Щ0 (75934
55 10h40m 10h36m +41 +38° 10h28m 10h32m M+7-22-25 ° i A1035 +40° °GS M+7-22-39 +39° M+7-22-10 •o M+7-22-29 <• 3237 •32 U5759 M+7-22-35 • 38 3304 о • о 10h24m ‘ M+6-23-12 M+6-23-16^ о M+6-23-14 10h20m URSA MAJOR M+7-21-44 °>M+6-23-10 TZ U5577 о U5563 1 Ohl 6m 1ohoom e 19 09*56" +41 10h04m 10h08m 10h12m LEO MINOR U5476 1.2557 U5540 3161 3159 3131 M+6-22-48 US391 I 0,1.2530 I +40° +39° M+7-21-32 ° M+7-21-29 °* I U5518 • .°. ' ,, M+7-21-15 M+7-21-30 M+7-21-10 0 • M+6-22-72 ° 1.2535 M+6-22-64 * M+6-22-68 U5389 +38° M+6-22-63 M+6'22'62 O' ИС101 TV 3294 +37° о M+6-22-51 +36° 0 3074 21 U5738 • 26 +35° 34 1.2542 +34° M+6-22-61 U5393 +33° LEO +32° 0 1.2561 о M+6-22-57 M+6-23-2 э M+6-23-1 3067 о | M+5-24-5 1.2568 4) 1.2566 M+6-22-73 M+6-22-40 M+6-23-15 1.2521 1.2524 . 37 3071 U5764 1028+313 +30 Rv LEO MINOR : 23 10h00m 10h36m 10h32m 10h12m 10h28m 10h24m 10h16m 10h20m 175427^ • о 3254 M+6-22-42 о i°n .’M+6-22-37 , +36° M+6-22-38 M+6.22-36 1001+292 10h08m M+6-22-67 M-^6-22-66 М+6-22-52 oo и5>382 <=* I I U5394 | M+6-22-45 U5349 0) •M+6-22-34 _________a. +37° • 29 1.2591 • 36 U5656 UU®« U5623 •27 . ™ •bUS622 28 1.2577 M+5-25-10 TX M+5-25-30 +29° 10h40m Io scale Galaxies 5-2 .U5490 U5474 M+5-24-22 3126° M+6-22-70 &.M+6-22-69 ♦ 3099 ‘ 20 3106 3116 \\U5364 : о Leo III 3118 £>---- +32° +33° +31° +34 О 2-Г < major axis U5481 U5478 о —p— 10h04m Galaxy Cluster to scale +30° 09h56m ОЭ^б" to 11 h24m +41° to +29° 0 LMI UMA, LEO WH 1юип / Barry / Wf„
56 +410h04m C ^4 ' 19 ' 7 T 09 44m °9h4°m 09h36m 09h32m 09*28m 09h24m 09^2С LEO MINOR LYNX 05389 Q 05193 M+7-20-61 +38" < 0 1.2516 7 05290 • 42 ___ -oM+7-20-31 M.,.°2M M'WS +40° ®16 •I M+7-20-50 05212 1.2493 о M+6-22-24 RSo ,40+39.25 M+6-21-69 M+6-22-4 . °' WO M+6'21'68 29710^2965 о h30223 2955 • M+6-21-58\* LEO MINOR . M+6-22-38 M+6-22-32 +39° M+6'22'6h M+6'22-62 05391 J U5349 I 4 1-2530 । ' -М+6-22-34Г V +37° 0 M+6-22-7 43 •ДЗС223./ ° U5184 05119 2922 ^.22-S2 : MV2'S’ 1 . ^."05382 “M+6-22-40 05394 / M+6-22-42 ' M+6-21-43 +36° k о M+7-19-67 М+7-20-9 о # M+7-20-1 . M+7-20-2 M+7-20-6 ° I 2853 a £F _* 2852 0 2844 + U4970 ....28^ L * ti+7-19-62* , ---;--------- 4. M+7-20-8 c 12468 ^1.2467’ + 1.2461C' ------- .4 31 30220.25 M+6-22-22 11 0 0 • S 3012 о ° U4988 +34° 40 a +33° 05146 2944 2970 ^2968- ф 2964 0 M+6-22-57 2840 0 M+6-21-61 M+6-21-18. ________ ° 3074 U4953O M+6-21-44 8 M+6-21-40 ’. 05020 M+6-21-36^ • 2859 05015 о 05011° M+6-22-12 _ \o ,2„. I ^6 M+6-22-61 2942 3099 20 0152-10 0946+301 151 1.2490 » 05074 05108 1.558 3032 10h00m 09h56m LEO CANCER 09h52m 09h48m U5364 ° Leo III 1.2473 0 US393 о 2893 U5326 °3071 1-2524 . 05070 J 1.2476 M+6-2 2-1] I ° M+6-22-9 M+6-22-16 I о M+6-22-10 о °TU • R M+6-21-64 Q> 1.2491 30213013 ъзооз M+6-21-42 M+6-21-51^.6^ ’ - '-i-Ty—^-2-05088___ ’ M+6-21-52 M+6-21-70 V M+6-21-46 ° 05282 i LEO -0.... U!2>7 сад.a M+6-22-6 2926 M+6-21-48 ^-2^23 .U497T2833i J M+6-21-38 m+6-2O32 ;o,2828--c 0 <? I Ц. M+6-21-24S M+6-21-33 M+6-21-29 , 1Л 2839 2829 0 ''4-/1 U4972 3011 I 3067 0 M+5-24-5 M+5-23-17 . 3106 +31 ° L: 0152-70 О U5272 о © EM 0 05281 о 05276 2981 ®-DR 2918 +30° M+5-24-1 +29e :leo minor:' . 10h04m Stellar Magnitudes (V) M+5-23-37 1/5/85 09h44m 09h40m ‘ 09h36m 09h32m 09h28m 09h24m 09h20r o.o «ndbr^htef 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars Variable Stars Amplitude Amplitude Amplitude Amplitude 1 0 mag. or less 2.0 mag. 3.0 maq. 4.0 inag. Q A X Nova Quasar Radio Source X-Ray Source Individual members are plotted if separation exceeds 60’ Copyright €) 1987-2003 Wittmann Sell. Inc.
56 09h20m +41° г.— 09h16m 2785^/ U4867 09h12m 09h08m 09h04m 09h00m 08h56m 08h52m LYNX M+7-19-21 +40° U4699 2838 U4871 U4950 • +36° , M+7-19-14 ° M+7-19-13 О U4704 1)4702 U4889 Q 1.2434 38 U4767 •o ’• 2719 2724 ° & 2719.4 2759 °M+6-20-26 .&M+6-20-30 M+6-20-31 1 ’ 2746 U4649 VU4635 0 O I M+7-18-59 08h48m -о—з М+7-18-50 08h44m 08h40m M+7-18-44 0 I 08h36m - — +41 M+7-18-37 M+7-18-36 ч +39° +38° A 1.2461 +37° I. - 2840 +35° +32° +31° +30° 0 *2782 U4872 ЗС2!7Л О ©их uv. « M+7-18-55 • 1 Qj i й M+7-18-57 M+7-18-54 U4513 U4498 n »---------0— M+7-/8-3/°- • +40° M+6-20-50 МММ N МММ . M+6-20-49 0 * M+6-20-46 J U4837 o. M+6-20-21 M+6-21-18 + 33° CANCER 1)4777 • о о М+6-20-20 4779/' 2823 7 2833 Р • 2828 р М+6-21-24 о <&> 2829 2779 М+6-20-48 о ° 2780 U4926 ) ♦ a ^2793 64 . M+5-22-27 o U4878 RS FY о 1.2428 •61 2796 t°U4831 1.2439 2827, 28261 „М+6-21-5 о У • -М+6-21-12 2770 I ° W7SZ О M+6-20-36 M+6-20-37 66 1.2445 C150-56 +29° — 09h20m 04869 L244i ! ° M+5-22-20 ‘2783 U4856 0 2789 5 0912+297 M+5-22-25 0 0 U4860 2766 о 721 CH® 094 6™ 09h12m 09h08rn 09h04m 09h00m Open Star Clusters । Globular Star Clusters and Asterisms to scale to scale Planetary Nebulae 1 >30” 30--10" 10"-5" о 2691 2704 M+7-19-4 CX •• M+7-18-53 O U4650 0 33 • 2683 +36° +37° +38° 59 G2’ U4531 C150-14 о 1)4660 +33° +32° +30° +31° » М+7-18-47 IQ> U4653 1.2400 *1.2401 M+6-20-4 ^+6-'9-22 1.2405 ° 0 JL M 2ooo U4614 + nU4621 M+6-19-17 2638 Bright & Dark Nebulae to scale 10’-5' 1)4572 +6-20-3 M+6-19-20 2649 ’ <4 U4558 M+6-19-13 LYNX +34 1.2421 Cl 50-50 C150- +6-20-1 ЗА 1 O’ • • ♦— — — -f- • • ♦ • • • • • 0 FT • - ♦ 57 • • • ^2679 • • • • 46 < • • U4559 “ 8 ° • i • C150-43' 1)4611 U4617 • • • ♦ • • • 08h56m 08h52m 08h48m 08h44m m 1.2387 M+5-20-29 CANCERJ 08h36m +29° Galaxies □ Galaxy Cluster lo scale 2-Г < major axis i to scale 08h36m to 10h04m +41° to +29° LYN LMI, CNC, LE0 ww r^n / tony Луророа f R(maklus
57 Amplitude 1 о mag orles$ Nova Quasar Amplitude 2 .0 mag jndbngMw top.ngh. 0987.2001 W^nn-Be^nc. Amplitude Amplitude Double or Multiple Stars 6.0 6.5 7.0 7 5 8.0 8.5 9 0 95 97 Individual members are plotted ( if separation exceeds 60 Variable Stars Radio Source X-Ray Source 4.0 mag 3.0 mag. 0.0
57 08h00m 07h56m +41° U4068 2476 +40° 2495^ +39° +38° +37° 07h52m 07h48m 07h44m 07h40m 07h36m 07h32m 07h28m 7 ~ vk. i LYNX ^3860^ <9 , °M+7-16-23 0754+394 oM+7-17-1 М+7-16-22 ©СК СМ0 °2484 +36° н--------- M+6-18-6 +35° +34° +33° +32° +31° +30° 07h24m 07h20^ __07116+4Г Й781 ; М+7-15-15 U3997 U3849 о 133976 2444 ~ М+7-16-15 — 2445 +40° - +39° ©СЕ ЗС186 21 о CF, б, U3887 : 1.2190 *. о U3944 о U3811 2387 +36° U3966 2424 Intergaladic - Wanderer- 2419 173822 65 U3837 _ _ 2 -1 +38° М+6-16-32' U3937 о М+6-17-9 • AURIGA © GEMINI 2415 + LYNX °'U3913 70 42214 80 Л U3833 62 р •> (148-21 U3904 С147-31 U4042 С147-51 GEMINI . А602 ; U4047 о < М+5-19-18 о V345 ‘’1.475 ‘'С148-19 ^3°-2435 с U3995 М+5-18-26 -23^ Тб-7 2375 2388^ о 2373 •238Л 2385 2379 U3879 C147-I3 М+5-18-7 • 339 U4029 °l 71 О о ’ V342 U4055 о . 1.2207- о М+6-18-1 Q U4132 • • • о ф • • • 1.2212 о 1.2211 • • • • • • • • - ° U4131 +29° — 08h00m 07h56m 07h52m 07h48m V348 о о С148-9 75 G Ф 1.2204 ъ 0 1.2203 1.2201 • О < ^2410' • • • • Castor 66 а 1 1.2196 о 1.2193 1.2194 О 99 о С147-48 <> О М+5-18-13 U3829 о 1.2185 (147-10 07h40m 07h36m 07h32m 07h28m 07b24m U3780 +34° из776' J +33° U3774° U3788 07h20m - - J +30° бГ U3777; +29° 07h16m Pollux 78 p Open Star Clusters and Asterisms to scale < 5' Globular Star Clusters ф Ф Ф to scale < 5' Planetary Nebulae ф- -Ф- -Ф- >30и 3040- 10’-5" <5H Bright a Dark Nebulae C?<‘/ □ □ ° * to scale 10 -5' <5‘ G< A) > S' to scale ilaxies О О о 5' 2 2' Г <Г major axis Galaxy Cluster ( 'i to scale 07h16m to 08h44m +41° to +29° LYN GEM, CNC, AUR iVrf Г/П0Г7 / Barry Ra/^papnii/ will Remaklut
58 07h24m +41° »£h20” _ AURIGA >33781 9* . * + 64 • । M+7-15-1S 07 12 07h08m 07h()4m O7hoom 66 +40° +39° +38 +37° +36 О +34° +33° ° 1-2185 +30° m J +39° +38° W8Z? п5 +37° (33811 +36° АС +35° (33529 34 е U3537 U3694 +33° + 31° RS U3728 ° (33777 +30’ AUR 07^1бт 07h04m 06h52m 06h48m 06h44m +40° 07h00 m *+34° •о <2147-13 » М+5-18-2 М+6-16-38 М+6-16-32 М+6-16-31 М+6-16-29 U3743 о- • 63 133703 GEMINI о (33829 С147-Ю (33788 +29° 0/^2401 V339 07h20m о U3742 1 __ • г 2333 о (33780 (33776 М+6-16-23 133774 46 Т U36920 О (33731 07>'12т ’07h08m Stellar Magnitudes (V) 1 ♦ • • (33593^~, • L M+7-14-11 • • • • 2281 • ,. и3525 <• U3510o' • • M+7-15-< > M+7-15-4 ?! I Q U3592 • 1 1 • • • U3601 • о U3S96 • — * •• ♦ £j_ М+7-14-15 И ♦ • • M+7-15-8 ' • • U3612 0 ♦ • • • • • .. • • 59 ОХ -®- ’ _ ._м+б-1б- • Ц' за 73 62 61 4% 60 • —— • -J м+6-16-14 •°М+6-1 5-8 ♦ • . м+6-16- • . • • • -• • • • ^M+6-16-4 ^U3615\ P 1.2175 U3664. М+6-16-11 М+6-16-12 • M+6-15-15 • М+5-17-12 oV336 U3631 '1(33649 О • (J3619 М+6-16-1 2291 2294 q 2289 ’ 2290 ^ 2288 • • • • о QX О °RX * • • • ♦ • • • ♦ • • • о М+5 • • > ®|$. а4б-з • • • ♦ • • • • • • • • • • • • • • ♦* i • • • • • • • • • • • VW . \ • о • * • • • • • • • • • -• • • • • • • • • о U3590 • • • • • оХ • • • - » • • • • • • • • • • м+5-16-7 • • U3536 • • • • ♦ * < -‘U3571 * С145-6 * ’ 28 GEMINI Double or Multiple Stars @ © ® Amplitude 1.0 maq. or less Variable Stars @ © ® (•) ® ® (S) ® 0 Amplitude Amplitude Amplitude 2.0 mag. 3.0 mag. 4.0 mag. 0m +41° 51» +32° +29° 06h40m ° Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" 30 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Copyright О 1987 2001 Willmann-Betl, Inc
58 06h00m 06h04m 06h08m 06h16m 06h28m 06h36m 06h32m mZz-13-з i 52 l|/’ • 51 V456o +39° +38° +37° +36° +35° +33° +32° GEM m U3475 +38° +34° +40’ +39° 05*56% —n +41 М+7-/4-6 40 uu U3390 CO M+6-15-1 U3476 VW о V406 о V459 OB 48 RT Sh2-241 +30 V394 44 К 06h00ni 06h04m 06h08m 06h12m 06h16m 06h20m 06h24m 06h28m 06h32m 06h36m +29 06h40m 06h40m I 1 0 AURIGA • • 0 W487 U3499 U3481 M+6-15-2 5 01/3479 WW +31° 06h12m 1 • • • • • • • • • • • • • • • • • • • • > • * 2192 • • • • ♦ V452 © .— • • • • • - M+7- 13-П • • • • • r ' • • • • • • • —• • • • • • • • • • • • +36’ V442 о V454 +34 +30’ . AURIGA +29° 05h56m Open Star Clusters and Asterisms f 1 f 'i to scale < 5‘ Globular Star Clusters ® ® Ф to scale < 5' Planetary Nebulae ф <> 4 >30" 30'-10" 10"-5" <5" Bright & Dark Nebulae <2?<.'?' □ ° to scale 10’ - 5' < 5' Galaxies 0 О О о >5’ 5’-2‘ 2'-Г <Г to scale major axis Galaxy Cluster *s to scale 05h56m to 07h24m +41° to +29° AUR GEM Wil Tinon / Barry Rappoport / Will Re так ho
59 06^04^ +41° 06h00m 05h56m 05h52m 05h48"i 05h44m aurica +39° +38° +37° +36°' Cz21 +31° m +30° М/ +36° v436 V442 V423 •э V419 +35° +34° v43 St8 18 19 +33° 834 8e 69 1985 +32° CQ +31° FU 26 +30° oHH V362 Be 19 1896 05h56m 05h52m 05h48m P178.3-2.5_____[ 410 17 Simeis 147 Sh2-240 ®V433 • 31 1) +32° Sh2-24l. +29° 06h04m U3390 CO • • • 1 • 1 • • • I. • 1 • • • King 8 = 2099 M 37 • V440-® • • V438 о Stellar Magnitudes (V) 28 29 T 1 •* I • ♦ 1 • • • • ~ — 1 9 ~T 0 U3325 ♦ • • • • 05r • • • ’24 4 Cr62 * 9 9 • 15 j •+41° • +40° •: i 1857 +39° • +38° +37° • • • • • • P170.7+4.6 _ _ • • • 9 9 9 —• • • • .. • ♦ (• • • • 9 • • • • • Cz20 • • • • • • • • • • • • ♦ • • • • • • \ • • • ~~ 9 • • V428 • • • • • • • ♦ • • • 0 <- ♦ V— L • w RU’ • • • StIO Y.’ I ♦ • • • • • • • ♦ • • • • • ♦ • • 2 ®V420 0 • • • I 1 V432 ♦ • 9 oW • • / / / Oe Pl 73.5+3.2 ____ I Sh2-235 Sh2-231 P173.7+2.7 1912 M 38 ©LY 1907 Be 71 . NO® v435 05h44m 05h40m 0.0 andbnghiM 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 80 8.5 9.0 9.5 9.7 8226 05h36m Double or Multiple Stars 19310 1960 M 36 > z V40b * <>V424 05h32m Variable Stars Amplitude Amplitude 1 0 mag or less 2.0 mag 17/ IQ®® 16 • • • • • • • • • ♦ • 05h28m 05h24m +29° 05h20m Alnath TAU Amplitude 3.0 mag. Amplitude 4 0 mag Q A X Nova Quasar Radio Source X-Ray Source Individual members are plotted if separation exceeds 60" Copyright © 1987-2001 Witlmann-Bell, Inc.
59 loq Cr62 V416 +40° +38° +37° oEO +36° V348 V414° +40° +38° +36° +39° +41° V419 05h16m 05h12m 05h08m 05h04m©05h00m 04h56m 04h52m 04h48m 04h44m 04h40n1 •* V593 uz 5 v346° AW AM 829 *4402 vdB31 v411 ^V3205 823 о vdB29 3C123 B24 V473® AURIGA TAURUS AURIGA .4-9.1 4 Ci) V409 "+30° +37° +33° +32° +29° +31° RX б*' —о V413 1852 +39° , .: King 17 TX ' 1.2120 0 V417 +35° +34°^ 19 Be 17 +30° AE •17 AR IQ® ® 16 +29° — 05h20m •05h16m Open Star Clusters and Asterisms to scale < 5* • • ♦ • • • • 4892 о 3C125 Pl 67.0-0 ЗС/34Л 1778 Do 15 PERSEUS <>PI66.4-6.5 Pl 65.5-6.5 1.405 flaming Star Nebula - +34 8222L_ 3C131 Pal 2 .8221 Skiff10507.2+3050 B28 Ц : 826 7bS2Z >< 8219 05h12m 05h08m 05h04m 05h00m 04h56m 04h52m 04h48m 04h44m 04h40m 04h36m Globular Star Clusters Planetary Nebulae Bright & Dark Nebulae □ lu scale Galaxy Cluster Galaxies to scale 5-2 О 2-Г < major axis >30’ 30" 10" 10"-5" to scale 10 -5’ to scale i 04l’36m to 06W л.id +41° to+29“ ™ +41° to +29° Гтоп / Barry Rappoport / WiH Яеггюккгь
60 Stellar Magnitudes (V) агхПх-ghtw 0.5 1.0 1.5 2.0 2.5 3 0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars Variable Stars n Nova Q Quasar A Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" О ® ® ® (•) ® © (•) ® О Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag 4 0 mag Copyright® 1987-2001 Willmann-Bell, Inc
60 04h00m +41’ r- 03h56m 03h52m 03h48m 03h44m 03h40m .. PERSEUS 45 E +40’« +39’ +38’ +31 +30 U2859 C.U2861 0Jb52«, О’”24” — '— ^2756-02742.• - o • о A I . Ъ, • J 02698 ^ 02686 •• •1J2766 U2752 u2730\s a U2689 U2736 »-T'- U2708 M+7-8-4 <aC54l-H 03h20m 03h16" 02617 . 1.309 02659 • vdB24 XY®~ о U2857 AB 1.311 M+7-8-17 M+6-8-27 U2810 03h36m 027987 +38’ , U2837 +40’ +39’ U2?i6 OU28VA * • U2828 ♦ M+7±25 ’ iw®- U2771 0 U2784 о • U2783 c. 02661 *. 02709 02685 V496 U2710 U2636 02702 U2633 1333 03h20m 03h24m 03h28m 03h32m 03h36m Д426 Perseus Clusfer 1.1900 +37“ +32’ 02653 M+6-9-4 U2808 M+6-8-15 +37’ +35’ +34’ +33’ +32’ +36’ • • • — -4 L' • • Californk ф Menkib 46; • • U2889 о 1 • • 3 1499 . i Nebula ' 0 U2881 U2885 .Q> ♦ » M+6-9 M+6-9-W 0 U2877 • • • U2868 . 0 • P156.9-13.3 -9 • • • ♦ • • . 1.351 0287 7_ • .AF • • • • • • • 4 • • U2901 9 • 1.2003 <> ♦ • * • ♦ • • ♦ — • •> 0 U2886 U2882 • 9 • • • • • • 1465 0 U2888 Ф > M+5-10-1 44 С ф Atik • X Per • • ♦ • • A 3C93J. 42 П (V467) 0 RX \ \ X ♦ • • • • • • V 9 i / • J348^ L. • • 40 о Л • • • • ♦ b~-. ! ! / у 84 ’ i i • • • ♦ i-,83 L- У'1 • • • • • TAURUS ♦ • • • • • • • • • • • • • • • I. ♦ • L 0 ♦ • • л-lh А ЛП U2807 +29’ 04h00m 03h48m 03h52m 03h56m U2780 1342 U2746 о I . 02706 о U2770 R • • • • • 02623 o 8206 B205 B204 Q vdBI6 B2O3 V574 B202 +36’ +34 V573 © U2629® U2627 PERSEUS ARIBS +30’ +29° 03h16m Open Star Clusters and Asterisms О О о to scale < 5‘ Globular Star Clusters фф e to scale < 5’ Planetary Nebulae -ф- -ф- <- < >30" 30 "-10й 10"-5" <5” Bright & Dark Nebulae □ о a to scale 10'-5" <5 Gel Ao >5' to scale laxies О о о 5' 2' 2' V <Г major axis Galaxy Cluster ' - X to scale 03h16m to 04h44m +41° to +29° PER TAU, AUR, ARI
61 03^24т +41° 03h20m 03^1 03h04m 02h56m 02h52m 02h48m 02h44m 02277 PERSEUS "V568 +40= 1.311 ° 02256 002185 1077A 10778 12 1233 q +39° 02709 57 +38° ® 02543 02636 1.1900 +36° +32° +31° +30° U266i e; q1.304 1.305 0 U2685 о • 02659 » •I 02698 02689 02686 . . 02708 03h’^ , 03h08m U2617 1.309 +37° 03h00m 'Л Star) 02546 ST 02243 20 16 о 02305 02328 b 02259 P 02169 AH +34° + 3 oV567 V574 02156 02221 +3 ARIES 03h20m M+5-8-2 03h16n’ 39 03h12m 03h08m 03h04m 03h00m 02h56m 02h52m 02h48m 02h44m 02h40m U2213 02165 ° 02 о M+6-8-2 ° S 1226 1227 102ЗА 1023 6 ° I • U26S3 02706 02678 02702 02633 02623 V573 PERSEUS 02629 * 02627 02604 О +29° 03^24m Stellar Magnitudes (V) / о 1.292 H 1.294 02463 28(0 • do £524-54 1207 ©V571 1 V569 О '<• 02526 02550 о . j 02540 1.1874 22 It <2524-41 U2363 о Q M+6-7-19 C524-13 1.278 M+6-7-15 A407 ’ 02491 I \ о 1167^ 02465 02h40' + 02180 о °V560 •9 • .. • M+6-6- 1058 U2494 . Z-O“> 902456 • • ♦ • • • ♦ • • V564 • • • о • ♦ • и 02466. U2435 О 24 02223 1093 ' A376 M+6-6-77 02179 1050 U2448^ M+6-7-24 0 02392 TRIANGULUM . P U2206 U2222 Г • ♦ • • 1 * • • • • • • • • 1ч24в1о- • • • Double or Multiple Stars 0.0 ж ж . Individual members are plotted «MbngMe. 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 80 8.5 9.0 9.5 9 7 I if separation exceeds ЫГ 21 LT © AO U2376 Variable Stars U2218 " 1067 1061 n 02201^^1057 U22*9 ЮббТ^ ^02174 1060 M+5-7-39 • 02197 Amplitude Amplitude Amplitude Amplitude 1 0 mag or less 2.0 mag. 3.0 mag. 4.0 mag и Nova Q Quasar A Radio Source X X-Ray Source Copynqhtf) 1987-2001 Willmann-Bell, Inc
61 /Tj 02h08m 02h04m 02h00™ 02h40m 02h36m 02h32m 02h28m 02h24m 02h20m 02h16m 02 12 ---- +41° --------- 01h56% _——ii +41 1003 I ANDROMEDA Ф UI855 VI796 о ° 02126 V377® .0 U2034 ° 01988 0 U1780 02003 * °O1993 ЗС65 U1886 О I023A ]023 *<R|___ +39° 1.239 —rj- • • oU2014 •M+6-6-47^ о <02069Q U2033 02067 Q>U2O65 *0 о М+6-6-43 U1972—о"|------ U1941 +37° ° 949 +36° U1810 U1804 01772 TRIANGULUM 02143 "2094 О .0. М+6-6-53 о ’ 959 • о 1)1976 U17S7 о ^-01767 01787 ' ' 01691 • BX- • • о • ♦ ♦ 828^ • • 01674 o °;.. 818 U1660 ‘ 1 Ul582 Q V373 801\О ' 797 ° ’ U1418 М+6-5-69 О U1493; • °/1179 М+6-6-12 I L ° *М+6-6-5 о .........°........ Ш721 8о| 58®, 834 о* ‘ ] ° 841 । *01650 О i • । АВ ° til 604 °U1474 . 56 g® ...V U1398 • • ’ 170 Ul 882.'1оМ+6-6-29 ~в*» ®‘ AF М+6-6-20 IО О° 01877 ---— М+6-6-21 01769 — о U1788 о «23-2 •°U1654 U14l6o М+6-5-73 о |.178 ♦ V37H ' °. M+6-5-74 " U1460 о 732,V Д11415 01919 I ъ U1865 M+6-6-7 Ш776 о U1701 Г 861 M+6-5-106 . U1651 о о М+6-5-90 M+6-5-80 U1459o AU1400 +36° 753^ М+6-5-63 о ...............' ' ' ’ M+6-5-61 A262 U1910 . о М+6-6-27 01800 о *01735 АС 01668 01666 M+6-6-59o. '°?,2 U2090 '8>15 U2105 r, U2077 <, U2015 U1581 од М+6-5-83 о о OR U2109 • 968 a b s 3C68.14C M+6-6-57 ’ I оЛ 1.1792 86 ,.U1685 02054 02131 0 02023 970 U2083 974 . ^969 9788,Л и-022- 973 .1815? 01857* ^U1826 9Y(| . M+6-6-4 1 O M+6-6-1 • °O1829 e 0 01778 • ♦ „890 7< • w 01821 a — • - 0 01805 М+5-6-1 __ - - Г М+5-6-7 U15O3 761 o’ 739 I 750° 738 25l^+33° ' • 740 -736 U1422-° I 01.1793 1.1789 0 H785J * 01729 784 о М+5-6-12 OU2156 ^1.1823 U1980 о M+5-6-36 *U1825 • dM+5±35t____ о М+5-5-52 01750 798 789, U’470 _£_°—783-F' • 785 °? ’ С505- о 3(68.2 02011 A • о 940 о о» U1963 4>01890 о*11 01924 о U1856 М+5-6-14 U1726 г»5 01682 0 | (504-22 •° 02116 1012 0 U2122 ARIES +29° --- 02h40m о М+5-7-5 . (505-17 О U2053 02h36m о С504-101 O2h32m 13» 02h28m 0 01896 001889 01696 ° 01690 6TZ U1596 U1590 02h24m 01792 . ___0_______хэ.--—------ 02h20m AD 02h16m 02h12m 816 8190' 02h08m 02h00m +29° 01h56m Open Star Clusters and Asterisms to scale < S' Globular Star Clusters ф ф Ф to scale < 5’ Planetary Nebulae -ф- < O >30" 30’-10" 10" 5" <5’ Bright & Dark Nebulae M □ о ° to scale 10'- S' <5' Gc Д) >5' to scale ilaxies О О о 5-2' 2-Г <Г major axis Galaxy Cluster to scale 01h56m to 03h24m +41’ to +29° PER TRI, AND, ARI Wil Tmon ! terry Rappoport / Will Remaklus
62 +33° +32° +29° 02h04m +41°h°42’_ 02h00m S2m 01h48m 53Т 01145° • М+6-4-36 М+6-4-9 01022 0521-2 +37° +36° +34° U1059 0 * 01418 +40° 0522-28 +39° V367 +38° 551 01251 +36° А174 + 35° с. U1086 0U1131 561 ь 01125 '.1675 536 5 ,342^ Uli 66 Uli 78 M+6-4-51 01269 0 I 0522-2* +37° 666 01212 0 0522-19 56^;.U1398 .. . Г м+б‘5.53 V371oM+6'S'730 U1476\i -S\- 772. J U^o o 5P 'H1257. 668 759 ' I Q -Л 209 ‘ M+6-5-18 “* 501)^ 01h44m OlNinm 01h36m Ul 40m v, jo Qlh 01h2gm • • r • U1070 • ♦ • • • m 01h20m -----7---- +41° '4£m+7-3-29 M+7-3-31 +39° OQ М+6-5-69 V368 8010 • , 797 . +38° 01493 J01474 * 01459 WDROMEOA 7530 *- 714^ ’ \ -M+6-5-63 710 XX M+6-5-6fer T^IANCULUM • Аб . ..................679^ "oM+6-5-45 1.171 ..688 o U1272 ' M+6-5-10 U1277'^ • 1 669 . U 090 • 01221 662 ъ 3046 01046 ч 653 • 01503 М+6-4-52 М+6-4-46 01161 M+6-4-44 1 0 YZ 0909 о U1088 «V363- М+6-4-5 Зе 798 789 0 1 735 о 739 ' * 7S0^ ° 738 ____751 L.733 01422.° 2'36 < r . U1234 6 M+6-5-5 0 621 . 634, - M+6-4-50 M+6-4'42- М+6-4-55 587 0521-74 01295 U1306 A260 L 1 • 701318 U12227 01152 0 М+5-5-2 U1213 с ’ '*0128 608 U1095 0 614 1.1718 . Б> ЗС48 a579 582 Ъ \529 ? • U 940 0 OU913 U975 0 1.1683 0 / • 0 523 -a - +34° ('M+6-4-N ° 0878 сV7'б!5]' 4l6'483’ оM+5-4-26 O.IWX7 C502-84 о ЧГ c z, M+5-4-48^ 4C+32.06 11690 528 513 ° y> °tU862 1.1679 ^(502.43 r-1.1677 „С502-44 + 33° 494 1.1673 Q S04 1.1689 M+5-4-68 M+5-4-72 ° ° 0 M+5-4-71 • Ъ 472 U901 1.1666 • А278 U937 M+5-4-55 U987 $ * (J959 01470 ^—783 785 о U1341 М+5-5-29 +30° 01359 ° 2а AA +31° ~ 769 02h00m 01h56m 804 . 777 01 'o‘ 778 01327 01160 01502 0lh52m Stellar Magnitudes (V) and bngh(r 0.5 1.0 1.5 2.0 2.5 . 0 j M+5-5 -9 *01311 01h48m 0lM4m 01h40m 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars 57/ 0 566 ---- 01045* 0 t/97 7 +32° М+5-4-70 Pinwheel Galaxy □ •I 592 (star cloud) 604 ». □ 588 СХ .01033 M+5-4-59 .......... +31° TRIANGULUM М+5-4-56 . 3042 01h36m 01h32m 01 h28m Variable Stars Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. . 3.0 mag Amplitude 4 0 mag °0934 01 h24m +30° !.1672O 1.96 PISCES ---- +29° 01 h20m П Nova Q Quasar Д Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" Copyright?) 1987-2001 WHImann-MI. Inc.
62 01 h20m +41’ r— +39° +38’ +37° 00h40m 00h44m 00h56m 01h00m 01h04m 01 h08m U522 M+7-3-4 U690 M+6-3-17 •BN U518 U529 11578°. +40’ +38’ . 389 393® • I *39" 00h52m 3LV.«00h48m 00*36" +41 EG® 32 M+6-3-4 V360 37 U V357 M+6-3-7 U444 218 . 272 oU748 M+6-3-9 RR U697 * M+5-3-29 U442 1.1619 1/465 о U384 226 • CL U355 1/646 U433 . 69 6 1/633 ° U381 233 .. о /.66 C500-80 U43l 338 U388 M+5-2-31 0 243 U632 00h40m 00h44m 68 h 00h48m 01h00m m U669 о о U629 V5 о 311 ©1/692* 0 374 i?Pl07S +36’ +32’ +30° +29° 00h36m 00*56" U5<11 O»42"’ 0 M+5-3-32 +31’ • л 3C34 1^g>J?VA71 184^ • зое *O U732 1.1636 410 394 4^0 407 <- ----------397 403^ 399-°q . ‘398^ ^+5-3-72»^ 'gQ U724q ;d420 1^4 °Л8 384 *76 U743 0 - ’ 78 U742 O U524 PISCES • ANDROMEDA 3C19 M+5-3-3 RWtC^ U484 U485 0 о 1/478 L/525 о • • 01 h12m 01 h16m • U ANDROMEDA +40’ 15-- M+7-3-25 i M+7-3-22 M+7-3-1 206 Andromeda Galaxy 224 M 31 о U831 ___0_ U822 U811 ‘ 1.1647* 425 1/755 ° Al 61 M+6-3-22 +36° '.Al 74 +35° +34°. 404 M+6-3-25 U809 Andromeda II M+6-3-26 .....Л? 443 • 1.1638 ° 1.1648- ° 449. ° •. . Q__________4 ^47 KA C A 3 7 • M+5-4-12 +33’ +32’ M+6-3- oV361 о U602 o U614 M+6-3-2 M+6-2-19 V356 M+6-2-170)u480 PS +34 M+6-3-12 Og-------- M+6-3-13 1 о M+6-3-10 C500-65 +33’ M+5-2-28 U841 °468 31.1666 M+5°-4-14 • 0 1.1652 U835 457 о +31’ +30’ 1.1672 о ъ 1.96 +29’---- 01h20m > A165 0 444 1.1659 c '1.1654 01h16m 287 о 266 <=> C501-56 о [U567 ' 29b U598 • 82 g ? U673 • • • M+5-3-74 О . • ♦ * • • 83T ♦ • • • • • • 01h08m 01 hl 2m U5 ""1 1/511° U548 0295 <5 U557 3-42' M+5-3-39 •о о M+5-3-35 262 282 M+5-3-7 M+5-2-47 o.M+5-2-45 C500-74 О 1.43 U542 о 0 1/556 . . Open Star Clusters and Asterisms О О о to scale < 5' Globular Star Clusters ® ф ® to scale < 5' Planetary Nebulae -ф- -Ф- < ♦ >30" 30"-10" 10"-5" <5" Bright Sr Dark Nebulae ° - to scale 10'-S' <S' Ge >5' to scale laxies Ooo 5 -2' 2-Г < Г major axis Galaxy Cluster 'ч 'i to scale 00h36m to 02h04m +41“to +29“ AND TRI, PSC Wrf Тюоп / Barry Rappaporl f WiH Remaklui
00h44m +30° r-~ 00h40m 00h36m ---0--- 00h32m 00h28m 00h24m 00h20m 00h16m 00h12m 00h08m 00h04m oohoom П +3C ° CS00-48 ° U12 <28 GN PEGASUS ANDROMEDA M+5-1-63 +29° .uw +29 A21 U12899 U108 U12897 +28° +28 U202 +27° +27 U127 . M+4-1-44 U12896 a U110 +26 *214 V347 C479-54 +25° L +25 +24° +24 +23° ANDROMEDA PISCES +21° +20° + 19° 0 108 0 U29 U221 о ° M+5-2-8 O 97 U12901 С500-74 о 1.43 , \OU147 C4 99-95 C499-97 6 • U157 U146 |o +22° M+4-2-46 * о M+4-2-45 ° O U152 C499-98 • I @^U215 SW LR C500-15 ' U469 +26° ----- U400 М\5±31 76 ^'M+5-2-3 U411 • | о 0 U398 1.46 V351- U50 Mi-4-1-48 +23 U11 +22 U6 +19 4G 18.02 52 V 164 +18 • Ul 22 00h04m •00h12m 00h08m 00h20m 00h16m Double or Multiple Stars 7 0 7.5 8 0 8.S 90 9 5 9 7 +20 m Individual members are plotted if separation exceeds 60" U393 о М+3-2-19 . U12915 t 0 U12914 s U14 M+4-2-30 I °U321 U242 U265 a- о U364 54 M+4-2-43 । 229 228 л M+4-2-47 M+4-2-50 00h44m ‘ A75' ° U425 00h40m >30E ъ * -U37L c- M+4-2-39 0 » °U367 U375 I U360 169 1.1559 00h36m 162 160 52 U310 U278 о ° U227 TU _p_ 4G25.01 М+4-2-26 46 • A43 00h32m Stellar Magnitudes (V) О • U248 ° 1)244 о U261 U228 0 U210 1.1544 0 1.1540 OU179 0024+224 00h28m 109 aoM+4-2-19 Alpheratz 27 -Щь f?l/95 21 a M+5-1-S6 U105c ° ‘ J N0e ...... о ° M+5 -1-47 * ; о U87 • : о U92 °22^ U69 U68 M+4-1-40 o U40 C4 78-21 26 | ° 23 U79 а о U13 • 85 .M+4-2-10 1.1546 \ 86,r 9'6^2^ 94 '° •93^ A 9081 80 79 I 1.1542 -.85 1.1543 ‘ M+3-2-5 о U223 _Q__ U197 Mi-3-2-1 i. Mi-4-1-46 ®BW U169 ’ Mi-4-1-43 NQo 42 о ___a. 89 Z 0 M+3-1-33 57 о U113 M+4-1-20 Mi-4-1-19 41 15* • C456-37 +21 U12900 • • 0 U53 • • • • • » U3oe • ♦ • 87 • • • ♦ • ♦ • • U46 • U31^ PEGASUS o U12893 00h24m Variable Stars • ® ® ® (S) ® ® ®®o Amplitude Amplitude Amplitude AmplAude 10 mag or less 2.0 mag. 10 mag. « Onwq. « Nova Q Quasar A Radio Source X X-Ray Source Copyright О 1987-2001 Willmonn-Bell. Inc.
00h00m +30’---- 23h56m 23h52m •o 23h48m 23h44m +29* +28° +27Q +26° - о U12861 M+5-1-8 * M+5-56-20 M+5-56-11 7753 7752 78 М+5-1-17 о М+5-1-14 . XL M+5-1-15 U12855o U12873 о 84 Ш@. +25° к——— +24° +23° +22° +21 0 ^7798 +20° © +19° +18°. о U12879 С456-5 U12886 * C456-6 PEGASUS +17° --- 00h00m о U12840 © U12803 7775 о • 0 U12835 U12839 7777 A2666 • 79 •о* 'U12755 М+5-56-7 ° 23h36m 23h40m ®KT C476-96 U12625 LM 23h32m 23h28m 23h24m U12657 ®V354 °* М+5-55-24 М+5-55-12 * I I M+5-55-9 23h20m _Ph1+3Q° _ Т —V3490 PEGASUS о M+5-54-56 U12530 М+5-55-7 М+5-55-10* U12557 5 -|___U12566- — — о М+5-55-14 . M+5-54-61 ----- U12482 +29° М+5-54-58 о U12470 M+4-55-28 о С476-66 U12591 . U12636 •• еоШ2631 о М+4-55-26 +28° 7624 U12646 7628 1.5298 C4 76-55 G С4 76-30 о 1.5315 М+4-56-6 м+4-56-1 ljC476-120 о С476-122 ^'VVI5342 °7740 7726 7720 М+4-55-47^ 7728 j. м+4-55-32 \ о °. М+4-56-14 q 7747 19^7765 ' . . 7747 • М+4-56-19Л 7765 U12823 0 ---1____ U12792* • BK U12791 • C478-2 U12804 о М+4-56-9 о 7737 /.5341 ° • U12733 7735 7741 ° 3 7745 W357 °V359 3C463 . M+4-54-39 +27° A2634 U12587 V362 о М+4-56-10 0 U12732 * M+4-55-45 M+4-55-44 о 7784 83 23h56m °7718 .° 7698 U12663 U12655^9 M+4-55-23 /7712 M+4-55-24 А2618 U126961 4355 3C466 U12731 81 Ф ® 0 7786 ’ 0 U12843 А2626 ^ 1.5338 ----о- U12764 ° U12844 О U12725 M+3-60-36 U12747 о M+3-60-29 Д 3C467 M+3-60-21 M+3-60-28 U12784 U12710 о — М+3-60-9 ° *U12682 —°Ш2681— М+3-60-23 U12707 0 М+3-60-31 7771^О^69 . ----7770 ------- M+3-60-24 23h52m 23h48m 23h44m М+4-55-2 +26° 69 о 7664 7677 <?° 7673 68 D 7620 3C46O 62 T «> U12490 _______•--- +25° 75681 +24° -----1 +23° <S) 71 HW 0 7678 О U12619 С476-34 1.5317 1A2625 +22° ®V352 7688 о 1.5329 о 1.5331 • 65 М+3-59-48 0 • I »•- М+3-59-49 C475-59 +21° 75 KS 23h40m » 23h36m C454-71 . 1.5312 1.5314 M+3-59-64 « М+3-59-58 М+3-59-59 ° 7681ъо М+3-59-60 +20° 23h32m М+3-59-51 о M+3-59-40 М+3-59-47 ---------- М+3-59-57 о M+3-59-46 23h28m 23h24m A2572t .+19» 7^ Л873788 7602 S? * Л7578А К97-'' 0 7572 J М+3-59-26 M+3-59-27 +18° • о . 7625 23h20m 23h16m Open Star Clusters and Asterisms ( ) ( ) C to scale < 5' Globular Star Clusters ф ф ® to scale < 5' Planetary Nebulae -ф- < + + >30' 30" 10' 10--5" <5" Bright & Dark Nebulae C?<’y' □ □ a to scale 10'-5' <5- Gi 7^0 > S' to scale ilaxies 0 0 0 5'2 2-Г <Г major axis Galaxy Cluster ; 't to scale 00h44m to 23h16m +30° to +17° PEG AND, PSC IVrf Ti/ion / Bony Rapfxiport / Will Remnkhn
23h20m 23h16m 23h24m +30° r- - 23h12m 23h08m 23h04m 23h00m 22h56m V349e PEGASUS I M+5-55-9 , М+5-557/ .U^° M+5-55-10^ o0Q(j]2SS7 +29° — U12566- J^^±6n . U12482 О M+5-54-56 M+5-54-61 U12430 М+5-54-58 о U12470 +28° +27° +26° 7624* o 1.1473 MU-54-39 C496-50 °. 0 . y ,~ MU-54-53 ° U12413 O7543 61 M+5-54-38 ® MU-54-31 О 7487 • MU-54-39 i„W U12515\- | о M+4-55-2 о 7628 oC476-30 0 . 1.5315 +25°------ +24° k— 68 V +23° +22° +21° 7620 3C460 Л < > 62 T 0 1.5317 • 65 MU-59-48 I & > M+3-59-49 ® +20° MU-59-51 0 + 19°. +18° +17° — 23h24m EZ /.5298., * U12490 C475-59 о • • • V339 U12310 Scheat 7420 cs • о 7439 MU-54-20 22h52m 22h48m • A2503 Г) o U12212 r U12190 Matar 44 22h40m 735Z_”+3( U12163. 43 0 BD +29 +28 QV° ’ ST +27 60 QW° U12303 KU U12272 @56 MU-53-14 ° 7527 0 U12352 7568 U12291 = 7436 ™1. U12293 ^ 7433^7435 o C475-41 M+4-54-23 ° U12334 _ _ . 7466 U12191 .al. . U12193 +26 V341 7539 © ОТ U12400 V338 7375 51 • М+3-57-3 С454-1 U121S8 U12265 GO М+3-58-13 U12351 . о • 1.5274 0 1.5282 0 U12278 U12326 О V342 C453-65 U12289 U1228i 75]6 о • U12200 -M+3 58-8 3C454 • 45 0 MU-58-1 7475 Q 7474 --------3------ U12333 • » M+4-54-34 0 7548 MU-54-9 U12233 Sadalbari • Ш 48 LI U12425 ©V336 47 Л MU-54-20 о 1.5258 U12390 .\.J489 •---------- M+4-54-27° U285 . MU-54-22 ~ 7415 о 7411 7409 о . QR +25 +24 (.5242 /.5243 <? -ВС +23 +22 +21 +20 А2572 MU-59-40 74 97ъ М+3-59-1 М+3-59-11 М+3-59-46 23h20m о U12347 •2 U12344 M+3-59-9 4° 3C457 • Cs • 7625 • 1.5312 1.5314 * * 1.5284 ’ 4C+18.68. ° — —< MU-59-47 7549 7Щ^7547--- 1^7550 Л 7598 7588 \ 7602 4 < ^ 75788 7558 1.1472 23h16m 23h12m 23h08m 23h04rTI 23hOOm 7597 - ' 7578A- о ° 7572 < M+3^-59-26 M+3-59-27 0 U12259 р М+3-58-5 • 41 4( +19 C453-38 7)-------------- U12258 22h56m . AF °5Х Д’ 3C453 л +18 22h52m о M+3-58-7 22h48m 22h44m PEGASUS 22h40m Double or Multiple Stars Stellar Magnitudes (V) Variable Stars .Д.К 0.5 1.0 1.5 2.0_15 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Amplitude 1 0 mag or less Amplitude Amplitude Amplitude 2.0 mag. 10 mag. 4.0 mag. X Nova Quasar Radio Source X-Ray Source Individual members are plotted it separation exceeds 60" Copyright © J 987- 2001 Willmonn-Bell, Inc.
22h40m +30° * 22h00m 22h04m 22h36m 22h16m 22h08m 22h32m 22h12m 22h28m 22h24m 22h20m OX о PEGASUS A 3C441 43 0 AZ +29° 23 oTW U11852 i 39 M+5 +27° +23° +26° +24° +25° +22° +21° +28° +29° ov M+4-52-3 M+4-51-15 ss Ul 2059 732 . HP +21° ° 1.1420 41 +19' +19° +18° U11944 7177 PEGASUS 7283 M+3-56-9 ©- 0Y U12093 0 M+3-57-29 7290 * . о +20° +20° Ul2066 M+3-57-10 U12038 M+4-52-J1 .. м+4-52-10 M+4-52-9 7316 % . M+3-57-28 I a_______________ 21h56m л - - +30° +28 +27° QR +26° +25° +24° +23° +22° GX ©. 7286 -52-13 7253 • n 72^A 8 U1°1981 й • • о HQ* • • M+5-52-3 M^5-52-2 • ♦ • • • • • • • <32 Ф • U11978 • Q> • • • • • , 0 M+5-52-6 • • • • • • • • • W+4-52-6 • ®PT • • • V • • 1 oC • • 4! 7224 о 1.5233 012124 U12084 Ul 2036 о M+4-52-7 241 U11860 . о OU 7339 °O7332 /.523/ • 25 OW U11924 о U12067 й U12015 28 Ul1905 M+3-56-13 о -52-1 . RXo • M+3-57-23 ‘ tM+3-57-19 ♦ * M+3-57-22 40 о 1 7324 U12107 7323 22h40m 22h36m 22h32m Ul 2050 22h28m M+3-57-2 22h24m 22h20m Open Star Clusters and Asterisms Globular Star Clusters Planetary Nebulae to scale Bright & Dark Nebulae □ >30- 30- 10- 10--5- <5- I to scale 7241 §*011964 22h16m 22h12m 22h08m 22h04m U11878 Ul1868 22h00m 21h56 IO' 5' <5* >S‘ to scale ilaxies О О о 5-2 2’-Г <Г major axis Galaxy Cluster О to scale 21h56m to 23h24m +30°to +17° PEG № Tmn / Валу Rappoport / WiN Remakkn to scale
65 22*104m +30“ 22h00m 21h56m 21h52m 21h48m 21h24m 21h44m 21*136™ 21h28m 21h32™ 21h40™ PEGASUS • CYGNUS □ V2166 +29° +28° +27° +25° +24° +23° +22° +21° +20 + 18 +26° + 19° 15 35 +17° U11769 10 К U 11787 RR LO • 7053 о +23° ’ 7137 +22° sw ® NZ о 1.1420 о OR +19° U11868 AU NY ociM+3-54-9 M+3-54-10 13 +26“ +28“ +21“ &3C432 21h24m 21h20m , +30’ .’OV UH 852 : C493-8 ° 7116 78 Ц Uli 838 UH 830 Uli878 7/770 PEGASUS . 17’ >— 22h04m M+4-51-15 ° VI1849 +29“ VULPECULA U117S4 C) 7080 . U11728 ° • ° UH834 Uli788 о ___ d 3C433 A ' +25“ О U11860 0U AW —© О .OP +24 0 M+4-52-1 RXo M+4-51-7c.e M+4-51-8 M+4-51-10 DX 12 Uli 793 »VX NV Ф- 1.5104 U11749 VUL +20“ 22h00m 21h56m • • -• • • • • • • • • • • • 9* • • • ^2141+175 • • - • • . о 7056 21h52m 21h48m 21h44m 21h40m 21h36m 21h32m 21h28m । +17“ 21h20m Variable Stars n Nova Stellar Magnitudes (V) Double or Multiple Stars Individual members are plutted if separation exceeds 60" • ® ® ® ® ® Amplitude Amplitude 1.0 mag. or less 2.0 mag. Amplitude 3.0 mag. ® ® O Amplitude 4.0 mag. О Quasar A Radio Source X X Ray Source Copyright О 19Я7-2001 Willmann-MI, Inc.
65 20h36™ +30° 21 h16m 21h12m 21h08m 20h40m 20h52m 20h56m +28° +27° +26° +25° • P72.7-17.1 +24° +23‘ +22° * +21° +19° +18° +29 +20° +24° +29° +17° 21h20m 20h48m 27 30 28 DY RU М+4-49-/ ® *33 +22° • V404 29 . MX ° M+3-54-5 iM. 20h36m 20h40m 20h44m 21h16m 20h48m 21h12m 20h52m 21h08m 20h56m 21h04m 21h00m Planetary Nebulae Bright & Dark Nebulae Galaxy Cluster о NS C471-4 • . •> +26° c M+J-53-/4 DELPHINUS +23° +20° +27° +18° +25° +19° +21° 0 U11682 Open Star Clusters Globular Star Clusters and Asterisms 21 h20m tno • .9 • • • • 0 • • • • • ♦ • • © . • • • ♦ • * -TW • • ° 7013 . • CYGNUS • • • • • • - ,•—• • • • • • VULPECULA • ♦ •- • • • • • • • • • • • • • • • • • •» • • • • ® ER ® ♦ • • 7052 • • • U11707 • • • • • • • • • • • • • • • ♦ ® • • M+4-50-7 * • о Uli709 • • • • • • • • • • Mi-4-50-4 ♦ • • • • • • 4 • • 20h44m 6960 Filamentary Nebula U11722 U11717 PEGASUS 011683^ to scale to scale V403 U11676 M+3-54-2 C449-2 to scale >30" 30"-10" 10"-5" <5" 7003 10-5’ ® BW RR 52 ®T V402 о U11608 +28° • U11651 —0— M+4-49-6 —-o---- 0 U11653 U11643 M+3-53-1 — V400 26 . VULPECULA U11615 EU Ф о MY . DELPHINUS □ Galaxies to scale major axis to scale 20h36m to 22"04m +30° to +17° PEG VUL, DEL, CYG И6/ lirvri / Burry RafjfjufWft / Will Remaklui
66 20h44m +30° 20h40m 20h36m 20h32m 20h28"’ 20h24m 20h20m 20h16m 20h12m 20h08m 20h04m 20h00' P69.6-3.9 3C4IO^r@V2116 <t>P68.3-2.7 +28° +27° +26° 30 +25° +24° +21° ’ LQ + 19° + 18° +29° Be 83 23 BE V400 6921 P63.8-3.3 16 28 Д 3C409 RU V383® <§> • 29. • *BF MX о U11582 © MV EU<s> 13VZ 20h44m 15 20h40m VO335 20h36m 20h32m 20h28m 20h24m 20h20m 20h16m 20h12m 20h00r 20h08m 20h04m 1.4954/55 □ Ro 4 FG° 6940 ---- + • 6853 1 Stellar Magnitudes (V) Variable Stars S ® (•) ® ® (•) ® ° Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. в Nova Q Quasar Л Radio Source X X-Ray Source VULPECULA ° U11608 . P66.9-5.2 Be 52 +23° +22° +20° MV 26 • V399 ©• Bp. VULPECULA \ 6905 -ф-- < MW^ P65.2-5.6 24 18 U11615 • © MT C447-5 2 SAGITTA • DELPHINUS : SAGITTA 0..... V398 V2103 ® 21 NU >QR 18 oDR 20 • ь • Cr416 <>P65.1-3.5 6885 * FC1 P60.3-7.3^ 6886 15 *>P64.9-2.1 V397 • Dumbbell N - +. P60.0-4.. 179 GN 16 П P58.6-5.5.Q P56.8-6.9 00 andboghtef 0.5 3.0 3.S 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60" Copyright 1987-2001 Willmann-Bell, Inc.
6( 19h20m 19h24m 19h28m 19h32m 19h36m 19h44m 19h56m 19h52m +29° +24° • 14 NSo VULPECULA +21 ° +19° +25° +24° +23° +22° +26° +27° 20h00m +30° 19Тзо° zoo. V1507 6834 . €• 19h40m •-V2086 19h48m V2091- +23° * 6853M27 • • • ф Dumbbell Nebula GH su ®V379 CYGNUS ®sv 0z4 P60.5-0.3 • AT 6823 6830 vdBI26 P59.0-1.7* V393 Ro 3 +20° +19° HT CV +18° P54.4-2.5 A 30400.2 j.Be47 Ro 1 ♦P53.2-1.5 19h16r 19h20m 19h28m 19h24m 19h40m 19h44m 19h48m 19h52m 19h56m 6a О • V341 V 6p I <>>53.8-3.0 я Foo print Nebula Mi 92 a I 6842 HH +29° +17° 20h00m Brocchi's Cluster (Coathanger) ' * ® 7 ’ 6802 eV389 RS ® • 19h36m 19h32m V342® .40+21.53 • • A • • Millisecond Pulsar \ Cz40 -oV2088 +28° +27° +26° +25° +22° H P60.0-4.3 SAGITTA 127 V396 Sh2-90 P62.4-0.2 12 (V395) V394c, • VULPECULA 6838 M 71 ®9QZ • Ha 20 ’ • 6839 Sh2-88 10 Ro 2 6820 13 VZ 8s Sh2-84 . &P61.8+2.1 P60.5+1.8 P60.4+1.5 6827 • •3 • • • • Ф” • PS 7.9-1.5 P55.1-1.8 + VI764o • • • • • • • * • • • • ♦ • • V909 •• • • ♦ • ♦ • Albireo . —/fit— ““ > • • • • • • • • • •®>6p • • • • • • • • • • ♦ • P61.3+3.64> .®V391 • V840 J +28° V473 + P59.9+2.0 + P59.4+2.3 . V392 л P58.9+1.3 U + P56.4-0.9 ® P55.5-0.5 + VULPECULA ©V390 3 (V377) LYRA P59.0+4.6 6793 2ES ^P56.0+2.0 • JSh2-82 P55.3+2.7 . ( ^P55.6+2.1 . +21° • 4 • <- • • +20° •* ♦ U Be 44 • 1 P53.3+3.O • P52.9+27 Pal 10 Ф PSI.3+18SAGITTA Open Star Clusters and Asterisms О О О to scale < 5' Globular Star Clusters ф Ф Ф to scale < 5' Planetary Nebulae <><>❖> >30’ 30--10" 10"-5M <5" Bright h Dark Nebulae D to scale 10'-S' <S' бг >s to scale laxies О О о S' Z 2'Г <r major axis Galaxy Cluster \ 4| to scale 19"16m to 20h44m +30° to+17° VUL SGE, DEL, CYG Wif Ttnon / Barry Rappapo/t / Witt Remaklus
Stellar Magnitudes (V) Double or Multiple Stars Variable Stars Q andb^Mr 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 I Cufjyrtghl © 1987 2001 Witlmonn-8ell. Inc. Individual members are plotted if separation exceeds 60’ Amplitude Amplitude 1.0 mag or less 2.0 mag. Amplitude 3.0 mag. Amplitude 4.0 mag. X Nova Quasar Radio Source X-Ray Source
6 94 V 18h00™ 17h56" 0 +30 18h40m +30° 18h08m 18h04m 18h36m 18h32m 18h28m 18h24m 18h12m 18hl 6m 18h20m . ? Cl 72*40 V976 * oU +26° +25° +24° +23° +21° +20° . +19° U11070 +26° +24° +29° +27° Cl 72-4 1127 6680 +22° - 1071 U1U94 105 о U11113 +230 • 97 AC oV990 96 0 V973 ®V889 +18° IQ V992 b 6555 U11107 M+3-4 7 -10 0 6548 % 6549 +20° +25° +19° +22° +21° Uli 237 ° V994 л6501 6500 о о ’ U11289 ° ,, >108 * M+5-43-16 ° wl • . Uli 162 • o' V815 +29° +28 +27° • a.l . • • • ♦ • о . Uli 307 • • ♦ • • • • • • • • • 6632°^ • • • • .O6671 LYRA • RZr— • • • -Ф-Р55.4+16.0 * • • • ♦ • • ♦ • • • ' HERCULES • 6674 0 • • • ___________ • • • V995 • л • • • _xSY 6661 °6658 Ul1285 V774 о U11246 ' U11261 6669 U11314 • Ul 1294 J M+3-47-8 v999 V993 M+4-43-33 M+4-43-31 U11229 109 <=> V989 -V998 U1I151J 18h40m 18h36m 18h32m 18h28m 18h24m U11179 Io 6602 0 . U11068 M+5-42-29 UU098 1030 U1J123 OU 6518 Ul 1090 0* > M+5-43-9 U11150 о U11142 U11156'° 6581 *U11155 ° 6599 .э 6628 6623 ,o a6619 • * ♦ • • • • • • ♦ w- 6616 0 6593 C142-19 6547 V979 M+4-43-4 U11197. V988o • • • • 18h20m +28° ъ '011060 111 1064 jU11082 M+4-42-22 U11097 *6513 Ul1063 .U11170 6577 . *'6580 ^4 ^6i76 6579 o .6571 V772 ъ M+4-42-17 6586 о 6587 U11152 V985 in? • U11120' 6527 0 V978 V974® RY C113-24 18h16m 18h12m 18h08m 18h04m HERCULES *0 V975 18h00m 17h56'r 4 open btar Clusters and Asterisms ОС О to scale < S' Clobuldr Star Clusters ф ф Ф to scale < 5' Planetary Nebulae -ф- -0- < >30" 30"-10й 10"-5' <5- Bright & Dark Nebulae <2?<C7' □ L'j о ::: to scale 10 -У <5’ Ci >5' to scale ilaxies О О о 5*-2' 2’-r ci- major axis Galaxy Cluster О to scale 17h56m to 19h24m HER +30° tO +17° LVB.VUl.SGE Wil J mon / Barry Ruppupurt / w>tl Remake
68 18h04m +30° 17h24m 17h28m 17h32m 17h36m 17h40m 171144m HERCULES V976 ‘V948 +29° -15. M4-5-4 OU . U11068 +28° +27° U11082 +26° U11097 +25° +24° +23° +22° +21° +20° 6527 0 0 6364 U1M70 V974® +24° +25° +22° +29° +18° +20° V978 +19° 4-21° □ RY M+5-427 »°V830 1Д2Гзо- M+5-42-29 UJI09g ---------1-- ъ U11060 Uli 064 M^5-42-14o • V965 • 78 ’ P5/.94-25.8 I «С140-25 79 • DoDz 8 U11063 V951 • C/4/-8 1.1269 °M+4-42- V950 V973 V656 oU10966 +18° <oV964 6467 HERCULES ©V975 4 17h40m 17h52m 18h00m 17h56m Variable Stars Double or Multiple Stars Stellar Magnitudes (V) 1 <s> A U10944 ’0 Nova Quasar Radio Source X-Ray Source 1.1268 /7204-246 ♦ 70 +26° +27° U10941 • 0 M+3-45-26 . & M+3-45-25 individual members are plotted 10A^g'ort, и separation exceeds 60 *_____ о M4-4-42-2 6427 _____________ +23° ‘ RS • -Г— « less 2 0 mag 3 U ______ 7° --- 18h04m 94 V 18h00m_ 17h56m 17h52m. 17h48m 7лр?6486 • U11017 6518 U11090 ** 0 U11046 P53.3+24.0 U11042 • M+4-42-22 0 • 89 (V441) U11043 . 0 U1 025 M+5-42-10 U10999 0 87 +28° *6513 U11027 U11029 ' 6484 • • o U11024 6482 f 95 96 6501 0 U11044 U11039 о 6490 • 6500 6495 V956 86 Ц U10972 6429 84 CF • v959® U10926 83 6417 U10928 /Р45.6+24.3 U/0894 U10866 0 6371 6372^ • 1.1256 76 X ; cи10909 и U10905 V949 1Л0837 I___________ ----00 ’ Ш0879 о> м+4-41-18 U10831 • • * • . U/08I3 U10840 ош0828 J 6458 6460 0 ° © V969 ГШ0979 4. ° 6452 6442 M+3-45-32 <3 Cl/2-4/ 17h48m M4-3-45-8 M4-3-45-3 0 AN M4-3-45-5 0 U/0899 A3C359 0 6408 p- • • • • ♦ • • • • • • • • •0 U10919 • • • • ,L_ 17h36m • 17h28m 17h24m 17h20m 17h44m „ ,0 » <0 05 —___—— -------
16h40m 16h44m 17h20m +30° f-- 16h48m 1 7h16m 16h52m 1 7h12m 17h08m 17h04m 17h00m62/4 16h56m U10673 I o- 6282° б^4Д M+5-40-14 M+5-40-25 Cl70-5 ’ +29° V944 +28 +26° +24° +29° +25° +27° +28° +30° oV938 V645 46 V94 3 ex V904 о RT 56 U10721 65 6 62 70 +24° V934 6243 U10692- +23° V903 U10787 +21° V936° +20° 1.1236 • +19° 54 +18< Cl 10-9 Cl09-35 ° oV915 • © V942 <=> 1.4624 16h36m •• Cl U10514 o +18° о 6321 1)10490 о HERCULES V928o +22° +20° (? 6308 $6314 M+4-4M -6315 1)10650 6276^ ъ 6278 •48 ®50 ° 6330 1)10658 -----0- M+5-40-23 ? М+5-40-24 о U10653 C169-12 626 J © M+5-40-1 +27° +26° +25° U10813 □ V832 U10717 •3> 63 (V620) 1)10672 ^ °U10702 I °V935 6272 6269 ' '~ 6270 6263 . 6265 6264 M+5-40-15 M+5-40-7 о 1.4630 6267 U10543 • 39 3C342 • ° q 16.4+267A,8 V926 V919 4 6228 Cl 38-65 V909 6233 U10528 6203 oo 6201 M+4-39-18 +23 °SY * U10 728 +22° M+3-43-9 Cl 39-22 —— +19 C110-10 о M+3-13-5 . V918 © C138-69 Cl 18-50 U10549 3C346 • -J +21° 17h20m 17h16m 17h]2m 1 7h08m 17h04m 17h00m 16h56m 16h52m 16h48m 16h44m 16h40m Open Star Clusters and Asterisms О О с to scale < S' Globular Star Clusters Ф ® ® to scale < 5' Planetary Nebulae -ф- < -Ф- < >30" ЗО’-Ю" 10и-5" <5" Bright & Dark Nebulae to scale Ю' S' <5* G< 7^0 >5' (o scale ilaxies О О о 5-2 2'.r <Г major axis Galaxy Cluster О to scale 16h36m to 18h04,n +30° to+17° HER M Ппоп / Волу Rqppoport/ W,H Remaklus
69 16h44m +30° 16h00m +30’ 16h40m 16h36m 16h08m 16h04m 16h32m 16h28m 16h12m 16h24m 16hl6m 16h20m +29° +28° +27° +26° +25° BE*! • 39 C138-7 о U10514 C138-I6 6148 3C336 Q M+4-39-18 V904 V909 о +24° j---------:_____ 9^6210 6203 * 6201 +23° U10445 U10351 . Q ^342 ®1634+267А,В V901 • U10455 P4 7.0+42.4 3C341. U10410 CORONA BOREALIS Cl 38-2 —19 ' A2175 C167-55 У 181) C167-64 HERCULES 6096 • 1612+261 о M+4-38-43 I Q U10262 о U \ 6086 0 \ 6085 0 AG AB 1)10151 +27° C137-59 • 0RU sx° 6075 6051 »V890 ® 10 LQ +24’ +28’ +26’ +25’ 6102 U1027. —Or— 6092 M+5-38-42 0259 ' A2162 6077 Г. 6076 • • U10250 +29° ----->:- C137-60 A2148 U10160 ®V903 +22° *6186 M+4-39-13 V900 ’ +21° M+3-42-19 +20° + 18° C109-35 HERCULES ? U10490 C 3C346 * 0 618 . M+3-42-18 I 0 * Cl38-50 4-19° k- 7O [ _ 16h44m 16h40m 16h36m 16h32m SERPENS CAPUT 44 Л о U10435 o U10211 Kornephoros 603 6052 U10153 C137-47 о U10232 & o U10297 16 e 6099 6098 U10138 : 0 : U10236 U10223 о ’ 6060 о U10243 ? • U10260 . о M+4-38-14 1.1156 j M+3-42-14 6168 О С138-12 з________ M+4-39-3 ° Cl 38-17 °U10413 • 18 +23° • 17 V894 20 7 M+3-41-137 U1O4O50 6084 3C334 Q 3C333 Д. 1.1178 6042 +22° +20’ +21’ U1012/ М+3-4Ы41 • • ' ' к o' о Л N C108-46 о; I о • • I 6034 о M+3-41-47 1 16h00m Stellar Magnitudes (V) V895 о о 6/49 16h28m 16h24m A2170 ; о M+4-38-45 U10321 М+4-38-44 6062 60628 4 ‘ C 08-165 16h20m 16h16m A2159 Double or Multiple Stars 6032 0 м+4-38-Ц глг-—h +19° R U10195 6061 2) 6057 :i08-138 5^60^- /6056 * 6044 \ '1.1182 ! 1.1183 6040 /Hercules Galaxy Cluster A2151 • : |< о ’ \ 6030 < I 5r +18’ 16h08m 16h04m Variable Stars 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 * ii Amolitudc Amplitude Amplitude Amplitude Ampliiuoc и 4 0 mag. 1.0 mag. or less 2.0 mag. 3-0 n Nova Q Quasar Л Radio Source X X-Ray Source Individual members are plotted if separation exceeds 60" Copynqhl © 1W-2001 Wllnvnn-M. Inc
69 +28 +27° M+5-38-6 16h00m +30° 141 +29° M+5-38-3 .AA A2142 6016 15h56m 15h52" . CORONA BOREALIS • 13E +26° Z° YZ SERPENS caput Cl 66-64 15h48m R® 1.4582 0 15h44m 15h40m m m 6001 ^6002 • • • • • Cl 66-23 0 • • - ♦ • • 0 5958 ° 14569 M+5-37-17 1.4570 о 1.4572 о ° A2089 + 15h28m • 21] 15h24m 15h20m 0 Cl 65-54 Nusakan @ 3 p 1 A2079 U9831 1 0 U9820 -A2065 Corona Cluster I5h16m —n +30° 48 X +29° +28° • • • ’л10 8 • о л « • • ♦ • • U10035 C136-36 о о C136-37 +25° . C136-62 M+4-37-42 5991 • . +24° PR +23° C136-43 U9984 1.4579 ъ 1.4576 0 U9954 0 U9999 U10073o U10074 1.4583 +22° U10059 A2107, ° U9958 A 3C324 Cl 36-50 4 U10062 О U10043 M+4-37-55 Cl 66-5 • +27° 5a RU Alphekka о 1.4556 CI36-12 A3C321 09859 О M^5-36-27 CORONA BOREALIS М+4-36-38 UV4> ° ' о M+4-36-46 • о 6020 U9927 0 M+4-37-14 0 1.4553 1.1*124 U9875 о M+4-37-4 $ 1525+227 , U9833 J U9825 0 • BOO i +26° +25° +24° +23° I +22° M+4-38-1 +21° _____________ C/f D v д 6027 Se7fer^ 6008B as,601 ^38 p o ci36-88 • Cl 36-99 o U10052 ®3C323.14 • +19° +20 M+3-41-4 ♦ 0 U10121 M+4-37-44 U10020 21 I 5975 о pq M+4-37-3 0 О C 1.1132 U9917 0 U9843 --------— I +21° "5910 z 3C318 +20° +18° • 5r ♦ • о м+3-40- 60 * 6003 —- <2 _ • U10084 • . • °° C107-53 U10085 • • °6004 U10050 0 • • 1.1142 0 ^>35 t • к • • 59 96 5994 • 22 Г . 1.1135 U9841 О о 5928 U9828 0 Cl06-26 </’ +19° A 3C3/6 •0 1.1151 U1OO93 . 16h00m 15h56m 15h52m 26 V® >A2108 M+3-40-18 о !5TJe +18° 15h48m 151144m 5977 0 5972 -0— 15h40m M+3-40-12 15h36m 15h32m 15h28m SERPENS CAPUT ’ 15h24m 15h20m +17° 15h16m Open Star Clusters • and Asterisms CO 0 to scale < 5° Globular Star Clusters ф Ф Ф to scale < 5« Planetary Nebulae c <> > * >30” 30--10" 10--S” <5- 1 Bright & Dark Nebulae Galaxies Galaxy Cluster j to scale —5 \ U L.J □ Ш “ •o scale 10*-5' 15l46mto 16h44m +30° to +17° HER SER, CRB, BOO Tnon / / W,N Kemakius
14h40 4 14h48m 14h44m I5h16m 15h12m 15h08m 15h04m 15h00m 14h56m 09831 BOOTES 48 7 +26° +25° +24° +23° +22 +21 +20° + 19° + 18° 5771 5773 °° ^29° uv M+4-36-38 +27° +28° 14h52m 1 0 5780 A2005 1.4514 A2019 о 09644 5827 .EX 41 CO 09770 45 c 5842 C134-63 EZ 09777 09620 09828 M+3-38-83 SERPENS CAPUT M+3-38-81 5829 о 09618 09596 о о С164-49 09594 о #5857 М+3-38-82 5859 1.1075 j£_ _ о С134-57 .09672 +4-36-2 1.1076 EQ A2065 Corona Cluster 1.1085 5778 о i .'A1991 л° 09622 09635 1096 I.1O97_ о e M+3-39-11 n c, M U970S M+4-36-16 . „ <2,1 +3105o 24m 15h20m 09820 1.4533 43 1|/ ' A2022 BOOTES CORONA BOREALIS SERPENS CAPUT М+5-36-9 о 3C315 д 46 b 3C310 0 Cl 35-36 M+4-36-10 09833 U9825о - 5910 3C318 OR 09763 M+4-36-23 С106-26 ^ M+3-39-14 3C316 .OS A2036 0 U9713 C135-J3 • 09718 1.4497 M+5-35-/8 .EP EM C134-33 M+4-35-6 о 09578 ^5735 EG 5737 1.1062 о 5760 1.1050 M+3-38-27 0 М+3-38-38 DE® EO; Izar 36 8 1/9544 o RY _®___ C134-38 1.4498 C134-24 5748 '° 09503 M+4-35-5 09480 14482 15h24m 15h20m 15hl6m 15h12m 15h08m 15h04m M+3-J87J 15h00m 14h56m 14h52m 09558 . о • 35 0 BOOTES 14h48m /J053~14h44m 14h40n Stellar Magnitudes (V) ?s J0 40 4 5 50 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars • • • Individual members are plotted if separation exceeds 60” Variable Stars (Ц®® @ ® © (•) ® ® ®>®° AmpMude Amplrtude Amplitude Amplitude 1 о mag or lest ? 0 mag 3 0mag. A.Omaq n Nova Q Quasar A Radio Source X X-Ray Source Copynjhlt) 1987-2001 W,llmnnn-Rell. Inc.
1 1 ЭЛ <25p 4h40m 14h36m 14h32m 14h28m 14h24m 14h20m 14h16m 14h12m 14h08m 14h04m 14h00m_ _ J3h5 1 . 70 6т +30° +29’ +3U >70 • BOOTES 0 о 5685 • ’ 28 a • • 5642 ♦ 5657 0 1.4442 ♦ 9 • 0 M+5-34-3 ‘ fu9l M+5 ♦ 135 :: M+5-33-47 -33-48 «о : U8999 °* : • * г X/FNATICI • > • • ©Cl М+5-33-41 С162-29 5 375 ° ' +28° • +27’ +26° ♦ +25° +24’ .j v 1.4479 о •EC • • • • 0 0 5641 C163-70 • • S' U9155 • • ♦ z " 1 \ ♦ A1873 z • 5466 i М+5-33-. о • сх ^8961 t ’8 1.4355 0 • o U89jl _ _ 1 > +28° J +27’ •— • • 1.4452 . • ° 4 • U9317 о 5635 • © 1 C163-32 О • • • • ) 1 о • .4384 • • • • 11е ^^'А1831 9« ! • ® R • ♦ 9 ( • Q 1425+267 • • ‘°U9. M+5-34- ♦ 5594 о *44 234 • о 1.4395 23 063-17 • l.4399o o 1.4397 15 ° ° 5553 U9101 ♦ • • • • • s 1407+265 • М+4-33-39 о • • о U8904 _ ZZ® 26° +25’ +24’ Е> *23‘ о U9418 • о 5677 A1927 DX®<5 56k 0U9 Q U9340 5659 • 1.1017 79 294 1.4418 —•— °UV | • • ♦ О 5548 • о 5523 5498 * о 0 1.4381 • 12d 1402+261 • а 32-6 ♦ 0 U8879 I 9 ’ _1 — •— —1 • • • о U9396 •AD •> 9 • 5610° 1 c , 5559 ♦ 9 0 5508 • C133-4 о ; I 0 U8873 ♦ 0 | 4132-64^ - I • • 0 1.4475 • • • 5637 U9322 0 о • 0 * 5581 • 1 9 • * Q • © • U9128 p • • • • • • • • • • • . -о +£ j +22°9 +21’ - +20’ - J • • • 2 6 • • • • • • U9138 • • • • • • • • • U9024 • о —“ • • •— М+4-3 • И7 • - + г; г° c U9401 • U9316 U9282 ° k • • • • • Г U9274 • • •o U918, • • ? U9164 • 9 • • Г4-33-44 о М+4-33 • • 40 • .U0OO7 1ое ' ©_ J +2Г □ 5702 n 5710 • M+3-37-24 * • 1.1021 • . • — • 5518 5513 • O o 550 • • • 9 * • • 9 • U8888 -г )а18-25 , О U8887 +20’ -8- 711 . . • • ♦ 0 о C104-44 • DZ © .Л ' oY • A 3C300 • • ® • • • 16a • • • (ф Arcturus ° 5492 • • • • • 1 ♦ • 4С+19.44 • • +19’ +19"0^ 1.4482 • • +18’ 1,0 U • О 1.4469 ° 11037 • • DY • • • U9212 CN • • "4 s— US M+3-36-93 • 090 /У84 q J9087 • - — • • • U88! • • Muphrk 0 8 Ц +18’ -1 +17' ПС6т • 9444 • 5628 ° • 1.4438 о • 1.441/ 0 • A1899 1.999 3.1000 U9167 • • 1.983 !^82e 5490C^ о °549 U9078 •- • а оз-8б • 0 • DP - — w © • • • 1.960 BOOTES • лИллт 1 Ч +17° *— 14h40 &• : e . iihnom 14h04m |4"UU m 14h36m 14h32m 14h28m 14h24m 14h20m 14h16m 14112m Wil Irnun / Burry Rupfjupuft I HW Rvnrukkn
14h04m +30° 14h00m 13h56™ 13h52m 13h48m 13h40m 5272 M 3 >5263 13h44m coo? ъ5277 Al 781 1 ’’ в 5274 \ 5280. 5275 13h36m M+5-33-41 M+5-33-38 U8961 BOOTES Al 831 M+5-32-56 9 11 • BZo 5251 1.4314 Al 795. M+4-33-39 ' Al775 = U8904 ZZ 1.4355 о ----0----- M+5-32-62 Cl 62-29 1 3h32m 13h28m U8483 U8510 13h24m 13^0" —i +3 CANES VENATICI 5375 0 1321+294s VZ M+5-33-13 A1800 +28 ° M+5-33-11 1317+27. Cl 61-85 +27° +2 +26° 1.4332 Cl 32-69 +25 1.4344 0 U8762 C132-36 +22° +21° + 19 0 5117 1.4234, о —b— 5116 U8788 Q 1318+290 °U8636 cxr--. - ° U8911 ^M+4-33-10 M+4-33-9 M+5-33-20 л M+5-33-19 +29° 1.4345 14343 о U8753 © 0 U8879 IO M+4-32-2 ° °DK 031-4 1.885 о U8598 о 1 о Cl02-41 U8507 Cl 02-67 °DL M+3-35-3 M+3-35-79 о U8839 о 5158 C102-58 1333+176 41 ° M+3 -35-27 14h04m 5190 0 U8701 o M+3-35-14 M+3-35-13^ BOOTES ‘ о U8703 U8705 ^5217 ° U8448 C101-51 M+3-35-35 U8409 5092 J4894 Oo U8535 KT M+3-34-28 о 13h24m +24° +23° +20c +18° oKS COMA BERENICES M+4-32-13 3C287 Q M+4-32-26 M+4-32-17 ° U8638 • (•) г 508 U8873 о Cl 32-64 M+4-33-37 U8889 IOS M+4-33-20 U8781 о M+4-33-19 U8888& • • -'Al 825 о U8887 4C+19.44 9 • U8850 1.960 1.909 '° FK 1.933 1.905 U8759 6 e • л 3C291 C132-9 M+4-32-19 +4-32-14 • M+4-32-12 о U8794 8П ф Muphrid U8516 5172 * о__________ • 13h28m 13h20m 14h00m 13h56m 13h52m 13h48m 13h32m 1 3h44m 13h40m 13h36m Nova Quasar Radio Source X-Ray Source Stellar Magnitudes (V) Double or Multiple Stars Variable Stars 6 0 6 5 7.0 7.5 8.0 8.5 9 0 9.5 9 7 Individual members are plotted if separation exceeds 60* Amplrtude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag Ю mag o.o and bnghtef Copyright © 1987-2001 Willmann-Bell. Inc
13h2Om +30° --- 12h48m 12h44m 12h40m 12h52m 13h04m 13h00m 12h56m 13hl 6m 1 3h12m 13h08m 12h36m ---, +30° U8025 U8076 M+5-30-87 +29° о U8069 842 5000 0 о 1.3990 UX. о 497/ 4944 О U8229 ^60o-14J 0 +28° ! M+5-30-108 4828 43 0 5032® 30 4957 C +27° 4892 ч M+5-31-153 1.832 0 +26° jlKHK IN P339.9+88.4 Mel 111 +25° о 1.860 +24° 5092 +22° f +20* +19° + 18° A 3C284 M+5-31-152 /> 4735 * 4738 5004 8 5004A Q> 4793 U7836 HH © о 5081 Ч Al 656 Garba Cluster M+5-31-45 0 4585 18211.818 b 1.4215 4842Af8 / wo 4827 b —W M+5-31 -95 , 4929 4907> 4 492 7 08290^ , 4854 +25° +24° +29° М+5-31-154й U8244^ 498} М+5-31-/4Г ° b G160-151 ° 1838 9 1.835 4849 4842 4824 OU8363 , ,, ° U8359 1317+277 4934 / 4921 о Q 4931 4923 ^0 4926А^ 4911 4926 Р49.3+88.1 О U8122 "4850 ° 4805 ' °’ М+5-30-101 • 48’6- 3C277.3 » : ° °47'5 4807А М+5-30-111 ^.4807 31 479Яс\ М+5-30-109' -;f о <^ 4728 о4788 } 4745 ^ 4721 ° 4789А М+5-30-116 * 4707 0 J789^_^ ' + . ov4821 4787 ° иоаоп М+5-31-18 • 4859 U8080 М+5-31-127 М+5-31-106 у4952 I I °4922 Q 49/1.4088/L8/l. М+5-31-140 0 М+5-31-133 о I Q 1304+295 М±31-[39О ^496^ 4559 U7890 1.3587 о 1.3582 * 4979 1.3581 +23 @ 40 FS 1.3736 1.3692 1.851 1.867 .862 M+3-34-3 о 1.4130 1.3721 4978 U8248 5053 42 a 36 25 38 32 0 1.3881 0 M+5-31-132° O 4961 41 h о 4960 +20° 1.858 c 1.857 + 18° +19° 4563 81 1.3585 ° 4556 4725 СОМА BERENICES °5052 Г 484JB 4896 о 4841А J J 4881 • ляле О4040 о'4851 а____________ —о. 1.4202 5016 4 ° 5012 M+5-30-70 ° 1.3598 0 U8343 KR«> +17 13h20m 1 3h16m 13h12m ® 13h08m to scale < 5 M+4-31-5 M+4-31-6 13h04m Blockeye Galaxy 4826 M 64 13h00m 12h56m North------------ Galactic о . lPo/е M+5-30-94 U8013 4692 467o 4673 b° U7959 q U7955 M+5-30-79 35 A1638 4747 12h52m KQo 4685 KP© 12h48m 1.3651 . о 1.3644 о • • • 4613 9 4615^ ♦ 4614 • • • 0 • 4565 4558 8+27’ О 1.813 1.3745 1241+176 • 4635 12h44m M+4-30-10 23 +22° +21° 24 COMA BERENICES 12h40m 12h36m Open Sldr Clusters and Asterisms Globular Star Clusters ® Ф Ф to scale < 5‘ Planetary Nebulae "ф- <> A >30r W-10 10"-5" <5" Bright & Dark Nebulae to scale 10 -5' <s Galaxies 0 I ° ° о >*» S'-2- 2'-r <!• to scale major axis Galaxy Cluster ; 'j to scale 12'36"to14*04" +30° to+17° COM B00, CVN Гюпп / Яо'ту Remakes
12h40m 12h36m 12h44m +30° --- 12h32m 12h28m 12h24m +29° +28°. +27° +26° U7836 0 U7890 /365/ 1.3644 о а 46/3 r Lyalls __ 1.3598 0 12h20m 12hl 6m 12h12m 12h08m 12h04m 12h00m --- +ЗС U7673 U7750 4585 4559^7 1.3587 о * °/35/6 — JJ559/555_ _ 4563 ®|9 455б . 1.3585° •’ о о 1.3536 4555 о 4495 °° 1.3441 IX О 43/4 /.779 ° 4253 ^4274 °4245 US6 4283 4310,, ОсЪ 0 4278 т, „ 4/73 те Box \ л • 4136 М+5-29-24 &4131 ’ 4132 1.3582 й U7017bo и7012 ©HY о U703I U7576 ъ 4448 ° . 15 у °4338 4375 о...... о 1.3309 1)7300 1.777 10 1219+285 о 1° s.4295 «n 423 ^7287 1.3263 о^УО*9 ° d 0 1.3407 * 4408 0 4393 о /.3243 “С — /3/65 «75 о /.3376 1.3421 0 14 U7221* <>M+5-29-35 4/85. 4/96* и " #4211 Ч 4211А IW ° х. - 4275 U7286 О - /3/43 GM о M+5-29-3 +29 О U7072 URSA MAJOR 4/04 •....... Q, М+5-29-15 M+5-29-17 4080 —о— +28 +27 16 * ° 1.3308 13 М+5-29-45 4146 а U7138 М+4-29-44 4614 4565 ^ 4562 о . 4 /780 12 . о 1.3122 +25° 21 о 22 +24° ° М+4-29-50 +22° ^1)7137 +20 о СОМА BERENICES 12h40m о I 1.3171 1.3215 —1.3203 • • о 1.3 86 KL 18 Me 11 23 4158 iU 1.3436 4293 24 4147 + 18° 4539 U7186 IY® М+3-31-61 4344 25 4450 , 12h32m 12h28m 12hl2m 12h24m I2h16m* 12h20m 7 0 7.5 80 8 5 90 9.5 9.7 о 1.3530 00 and bnghlet U7263 о 4561 Я 4336 1.3391 01/733/ 4766Г' 4155 U7133 -2-----О~ °U7I7O О4204 1)7321 1)7357 • U7270 1)7224 О 4455 I /79/ 4394 О 4382 М 85 0 4494 1.762 о М+4-29-32 с М+4-29-45 о о U7217 +26 +23 +21= U3692 7° - 12h44m 4635 /358/ М+4-30-10 Л ЗС274.1 12h36m IZ° 20 М+4-29-48 137266 ° 1.3075 '4101 -U7040 -4162 М+4-28-123 01)7141 U715/ 4 U7115 07143^ , М+4-29-37 ° М+4-29-38 М+4-28-121 о M+4-29-4 +25 +24 +23 С128-16 ---о---- М+4-29-13 • 1 +22' 4529 U76971 Stellar Magnitudes (V) ° М+4-29-2 2 М+4-29-12 4084 +2Г М+4-29-69 о U7346 О ОС99-/6 ^3-31-94 U7399A • • о М+3-32-3 © М+3-31-49 ---------О— 4098J.4^L 4^-ТП7 4070 4092 4074 о|,4060 4056 аля/ ^^4061 4086 4076' 4032 о +20 R • 41W 4064° U7074 в о "707i • U7100 М+3-31-41 ---—-о------- 12h08m М+3-31-29 о 4053 ^4049 4048 GK® +19' . +18' о0 М+3-31-15 4040 М+3-31-28 О 12h04m 12h00m Double or Multiple Stars Variable Stars ® ® 0 • Ф ® (*)® ® Individual members are plolled if separation exceeds 60 ‘ Amplitude 1.0 mag. or less Amplitude 2.0 mag Amplitude 3.0 mag Amplitude 4.0 mag X Q Nova Quasar Radio Source X-Ray Source Copyright О ^87 2001 Wdlmonn 8еП. Inc
72 12h00m +30° --- +29° Hh20m 1 lh24m I1h28m 1lh32m 1 lh36m 11 h40m 11 h44m 11h48m 11 h52m 11 h56m '<41213 3964 M+5-28-44 FX< M+5-27-89 U67910 3830 3912O U6883 3902 M+4 1.7460 U6806 M+4-28-45 3798 U6847O ° U6751 U6782 3761 3900 -0- 3944 0 0 U6425 06548 • 0) 06853 о 06593 4С+29.45 Q! 1147+245 1.2956 о • 06645 о 06861 06544 06476 о . М+4-28-92 3830А о 3826 .о 4002 • °4ооз с М+5-28-41 М+5-28-40 *3971 , 3984 3983 ° +28° +29° пы6;!0. М+4-28-36 °1.739 ’о U6846 о ° М+4-28-87 3951 3784 а^81 -м+5.28.з 3920 о -39)) 3814 ,в,, U6674 0 3812 3815 Q- 3629 о M+5-28-71 .0 U6325 3728 3670 oFO *° M+4-27-34 ° 3710 M+4-28-16 A 3C263.1 3926A 3926. 06301 о пг 4015 +26° +27° о 3832 3808 3808А 3748 3754 3753 / М+5-28-32 о U6761 3609 ОО 3612 М+5-28-11 Pal 4 URSA MAJOR U6292 => t М+5-28-67 иб968''^4008 U6637 3714 3712 ® М+5-27-79 о3713 oFT +28° +27° +26° U6522 M+5-27-68 o U6334 U6322 ..... M+5-27-52 h LEO 3678° io *3988 4004 4016q 4017 4018 4009/Згоо 4022 4021. +25°4023 +24° +23° +22° +21° ( ,<• М+5-28-13 М+5-28-15 о M+5-28-20 М+4-28-32 -------- -28-31 С126-101 3739 M+5-27-74 U6421 О М+5-27-70 . 1)6415 A1267 U6508 M+4-27-57 3689 1)6414 4 M+4-27-25 +25° 3765 о 3744 о 3772 М+4-27-72 3701 о U6509 ° М+4-27-53 U6976 S> . о М+4-28-117 о М+4-28-116 ° М+4-28-115 о М+4-28-65 3925 М+4-27-7 8 \ М+4-28-77 3940 о а. 3910 о М+4-28-33 Copeland's Septet 3745 Р 3746--------- /3750 3751 И 743 '3758 ’ и6495 М+4-27-46 о I 3954 о 3947с 06876 * 3929 М+4-28-70. I °/.742 0 С127-55 М+4-28-48 92 U6607 о 1.707 M+4-27-39 3697 3651 б> 3653 +24° A 3C256 3618 *3615 М+4-27-17 оо U6333 1116+215° • 72 FN +23° +22° 0 M+4-28-47 U6719 ’ Г C97-138 i384' U6881 +20° 3919 <5 3937 3943 U6821- 3883 О 06725 3884 Q / □ FY +18° ° U6891 U6741 о COM U6913 ----- в* М+3-30-115 д 3861 % Y 3886 ° $ I 3875,73' / 3862 L 3860 °й 3857 М+3-30-Ю8°яЪз859 '> 3868 i 3864 I оЧ 3867 М+3-30-113 .3821 3895 '0^ * М+4-28-29 3840 Q с 3816 r-fsWtar 3837 м+3-30-55 ° 1.2951 /А1367 3834 У о => 3827 М+3-30-49 ™°U6670 о U6687 +17° 1 12h00m LEO _____а 11 h56m llh52m 11 h48m 1lh44m 787 О U6609 е м+3'30;26 м+з-зо-21 * 06625 С97-36 о 1.701 M+4-27-36 о . о 3650 о U6332 Zosrr 68 5 « о 06525 436583 С97-П М+3-30-14 • 1.700 О М+3-29-61 о М+3-29-58 М+3-29-55 0 М+3-29-60 0 FV1 86 A 3C258 <5 06437 3649 0 3646 358 +20° М+3-29-34 °. +19° 3639 U632O0 О U6324 M+3-29-27 3626 3608> м+3-29 3607а 8 М+3-29-24 о о и6^96 . 3764 3803* /97-35 Оо I 3768 3806 о- 790 3802з801 3802 38 М+3-30-38 0 М+3-30-44А -----•— U6631 ,,136614 1lM0m • о « 3659 1 • 71 U6483O о3^6 * . , 3684 — I.2703 ° М+3-29-25 I 3602 Р 11h36m l/32m 11h28m 11h24m _ -J +1 11*16" Open Star Clusters and Asterisms \ / \ 7 to scale < S' Globular Star Clusters ® ф Ф to scale < S' Planetary Nebulae -ф- -ф- Ь >30" 3040" 10"-5" <S" Bright & Dark Nebulae □ L-3 D ;; to scale 10 -5' <5* Gd A >5 to scale laxies ООО 5-2' 2-Г <Г major axis Galaxy Cluster to scale 11h16mt0 12h44m +30° to+17° IVrf Гкю> COM LEO, UMA / Barry Rappoport / Witt Remaklus
73 4 +; +30° — — — —__ J1h16m 11h12m Jlh08m 11 h04m 11 h00m 10h56m 10h52m 10h48m 10h44m 10h40™ 0° URSA MAJOR • • . U6292 29° 2 О ' }А1213 * «* U6198,. • U6220 . м+ °U6152 LEOM 5-26-46 0, • ♦ IN0R ♦ • • • о U6031 • 43 • • • • М+5-26-2 • • • . . - +; !9° [-31 28° • О U6334 356 356 2552 < А Н 85 А 7~-Г,'^'255О 1 1 > 0 з. 54-^ 3553 • Leo A Cluster °3510 3486 о 06102 • 135/2 • • • • • • o3. • O 3400 3418 Yl O • 44 0 180 "м+5-26-4 15903 L UW о м+5-2. J5844 •• + 539 U6166 ^13527 . LEO l/jo-j/ 3558 "з 536 1 68 Mi 5-26-58 • 3515° М+5-27-52 8 М+5-27-1. ' 18 1 о М+Ь-26- +2; '°0- • • тг4 U6250o .♦ 3574 06247 • * • — 4 3570 06138 3504 oVV 3493 • М+5-26-3 —° 34 4 M+5-26-29 e 45 ^ 3451 lo ’-о—• 0 0 1/5927 1/5958 • их0 М+5-26-3 • • • г 4 -27° +26 J6415 ° 3629! о^609 3612 3< •е • • • 63^3563А 0> U 3534 о • -J 6190 • • 0155-46 • • • • • M+5J6-27 © UZo M+ U59/2oO • M+4-26-9 • 5-26-13 ° U5884 3 (15894 U5855 1.2598^ • <40 < +26° +25' M+4-27-25 • • • 1 • •0 U6325 • J • • U6252 • • • • • 51 • • • • • • • 50 • 48 • • • • ’° ^С/25-5' U5881. 3323 • 0 +25° +24° ^U6414 & 3651 3653 * • • ЗС250^ 67-е U6207о ’ U6204 М+ М+4-26-2 4-26-27А о • 7 М+4 • • 26-23^ ’ о 3475 • •~54 ♦ 334^ • • • ♦ 0. • _3327< +24° *23’ • ’ 1 3618 A 0 3C256 *3615 M+4-27-17 — • • U6246 ь ® 72 FN • 4+4-27-1 . 6А • о U6173 •п М+4-26-32 U6163 • ♦ • • • ♦ • LEO MINOR • • • • 1 • 15830° U5825U 41 • +23° +22° • и< оо 5333 ° F0 U6301 о • С126-1 U6253 , 4 •• /-• Leo II * ; FL о I U6194z‘ » 0125-30 • 0 • М+4-26-26 ♦ • 3437 • ♦ М+4-26-7 о 33 , 0 '^1100 Ч63 LEO 52 • • - +22° М+4-27-36 +21° - • 1116+2 • 15® . U6258 • о 3555 О Л Al 177 §06176 • • • ♦ • • • • о EZ • • M+4-26-20 0 U5924 М+4-26-12? о U591 M+4-26-13 О М+4-25-49 М+4-25-50 М+4 • • • (15805 ° -25-47 ^С124-. U5822 L/5801 >4 - +21° ♦ +20° - • ъ 3650 3649 ° Ъ 3646 • I U6332 ( • Zosma 58 5 ф' 3588 । • • • • 3522 . О • • 60 b • "^M+4-26 • • • •18 • • ♦ • • 0 U5833 - +20° + 19° -i М+3-29-34 °. • • 1 • • с 1/62/9 о • 1/6/87 • • о 06151 • • • ° М+3-28-54 • в • • • U5989 ° • 0 U5947 EW. • ♦ — +19° +18° — 3639 ♦ У65200 о М+3-29-27 ! U6324 J 3626 2608 М+3-2 0 О -3607^ ° 9-18 । 3599_ • • • ^(76/7/ 06175 3507 о • • M+3-28-29 • • • _ C95-51 <=>3426 ♦ • 51 m М+3-28-2 С 1.642 • “1. . ; *С94-10 5 —? +18° 36. • .LE +17° • 71 • 0 • М+3-29-24 о с3605 1.2703 ° U6296 о М+3-29-25 С 35 02 > ° 3592 98 • • • °’M+3-2f 0 06157 С95-104* —0 350/ 1-56 • ’ о 3487 М+З-28-52 М+3 • • • -• '28'45. 3473 U 3474 ® 0.95-7 3457 5445 ° 0 R 3454 6035 g3455 0 ° U5945 • • 3370 0 • • — +17° 11h24m 11 h20rT 1 11h16m 11h12m 11h08m 11*0 4т nh( *<+ Q )0m 10h56m 10h52m 10h48m /6'39 1 0h44m 10h40m
10h12m 10h16m 10h20m 10h36m 10h32m 10h24m 10h28m » юМот +30° ।- 10h04m 10h00m 10h08m LEO RV LEO MINOR TY 23 1001+292 +29° M+S-24-11 о 3265 24 • U5749 о US 621 +28° о 3274 39 • C154-21 +27° ъ 3251 +25° 3270 +24° +23° 3177 +21° USS09 +19° 0 324SA 03245 o 3277 о M+5-25-16 U5598 о M+5-25- о М+5-25-28 3235 3232 U5679 О I +18° +26° U5427? +20° +28° +25° 1.2598 Q 3254 09Ч6»0. °Г 1.2590 3196 ЗС240 1 о 3098 oDH UY ^3248 EO . U5691 3213 • 1/5359 3131 1.582 LEO XY •ET DD 3154 10h00m 0 3221 U5651 о M+3-27-14 U5552 <5 О U5672 М+4-25-34 ---------а U5709 • М+3-27-61 о о™” „ М+3-27-63 +20° +23° 0. ЗС242 1.610 I о М+4-25-14 - — +24° М+3-27-28 _ 3226о о 3227 3222 4 . М+5-25-9 О U5638 U5499 +26° U5713 1.2583 О о----- о М+4-25-28 ^ 3209 30234 о 3068 +29° 0 U5340 1.2520 ° --------- +27° °3323 U5588 1011+250 6 3327 U5710 U5683 M+4-25-19 /.2551 LEO +22° (- • р U5801 3301 3303 С94-98 о° 7» I-- 10h40m 10h36m 3216 3C241 C123-9 36 £ Adhafera 39 IU5498 M+3-27-1 ‘ 0 3162 US420 A p 3088A 30888 М+4-24-22 ^U5524 о I ° 3193 Л, 3190 J'87 3185 0С123-31 U5489 JJ5696 U5690 °- о | U5675 40 U5467 о U5431 ъ • о • U5434 U5436 U5403 . +21° U5341 А U5339 +19° М+3-27-46 о» 10h32m 10h28m U5639O о С94-39 3239°_____ 10h24m 10h20m USS 14,. 10hl 6m 10h12m 10h08m 10h04m AL- —1 + 09h56r Open Star Clusters and Asterisms О О о Io scale < S' Globular Star Clusters ф ф Ф to scale < 5’ Planetary Nebulae -ф- ф < >30’ 30"-10" 10”-5" <5’ Bright & Dark Nebulae c?<';7 □ O □ to scale 10 -5' <5' z^b >5’ to scale ilaxies О О O 5-2 2-Г <Г major axis Galaxy Cluster to scale 09h56m to 11 h24m +30° to+17° LEO LMI, UMA Ttriun ! Burry BuppufMjrt / W4/ Remukkn
10h04m +30° r- - 09h24m 10hOOm 09h56m 09h52m 09h36m 09h48m 09h44m 09h40m 15 f 2893 1.558 09h32m +29°^- 1001+292 30234 U5219 LEO 1.2520 о DX 24 Ц 0122-56 C122-80 •13 Rasalas 1/5084 0 3068 U5340 09h28m LEO MINOR +28’ +27° +26° +25° +24° +23° +20° +19° +18° 3098 <>DH 023-9 Q 0946+301 • 3032 • • 0 • 3026 • • • • DU J U5185 — ’/.2476 L <*- • • .EO 1 1/ ♦ 0 5040 ♦ ' U5002 ° • • • • 2862 0 09h20m ------, +30° CANCER 22 g U5246 о 17 E o° U5313 U5320 +29’ 1.2495 1.545 U5094 12 °U5129 °l.2486 +28’ 0 о 1.2490 U5108 U5070 bU5074 U4994 +24 2896 2885 Alterf 2931 2930'% -Л 2929л. +23’ U5005 M+4-22-52 0 I J122-/3 .EH 0)4940 2824 Г +26’ 2927 Г ° 4 X C/22-6 oEN +22° 2991 2988 EO 2916 V» • 20 DC ° U5192 +21’ U5403 +18° —cr~ 1)4985 о * C121-6 U5420 2994 о +20’ +19° +22’ 3088A 30888 I - +21° EC AL 1.582 092-62 092-58 09h20m 09h24m 09h28m 10h00m 09h56m 09h32m 09h52m M+3-25-4 o| M+3-24-46 I 10 ’ C/22-85 C;22.73 0122-37 2903 U5359 ° U5035 : M+4-22-32 : о . bU5341 0 U5339 092-61 3040n U5330 092-46 1/5/23 M+3-25-7 1.2487. 0 U5009 __________a. Q 0923+20/ • U5023 091-91 2843 M+3-24-5J M+3-24-55 XY LEO +17°------------ 10h04m 09h48m 091144m Stellar Magnitudes (V) 50 3.5 4.0 4.5 5.0 5.5 6.0 2943 t6^'^28 09h40m 2933 09h36m Double or Multiple Stars Variable Stars Individual members are plotted 6 5 7 0 7.5 80 8 5 90 9 5 9.7 it separation exceeds 60 Amplitude Amplitude 1.0 nug. or less 2.0 mag. Amplitude Amplitude 10 mag 4 0 mag. H Nova Q Quasar Д Radio Source X X-Ray Source Oopynght О /98 7-2001 Willmonn Bell. Int
08h44m 08b40m °^6+30’ 08h48m 08h52m 08h56m 09h08m 09hQ4m 09h00m 09h20m + 30' +29° +28° +23° M+5-22-20 09h16m . 09h12m •2?83U4856 ^2789 i' 0912+297 M+5-22-25 0U4860 о 1.2446 2766 721 CH о о 1.2443 3C213.1 0 M+5-22-6 1.2430 70 3C210 C150-14 C150-50 CANCER C150-48 Cl U4698 °U4611 2619 53 BO r U4591 • 1.2393 M+5-21-1 q C150-43 ^U4617 • aso-зо +29° +28° 58 p2 • M+5-21-5 • C150- О • • • • • Ф • A692 ( ) • • • • • • 9 • • • ♦ • U4602 О U4597 1 о 2623 U4940 M+5-22-34 +27° 75 • 1.2435 2824 +26° M+4-21-7 +25° +24° +22° 2764 +21° 3C213 +19° 2843 ? +24° +26° +27° +25° +20° о U4895 • WY 2753 Cl 2628 о U4592 UV 1)4643 о M+4-21-13 U4809 U4853 • 35 °. C90-4 1.2399 M+3-24-38 80 M+3-24-24 0 C9O-33 •78 ®X CANCER 08"40m 08h44m 0 1.2454 2794 0 2791 о U4828 1.2423 о О 0851+202 2711 +20° +22° 2790 U4858 c o M+3-24-29 T TX U4532 ' 0839+187 « .. 1.2392 • 2 774 “ M+3°-24-2 ____+2Г C91-55 2809 \<^2804 28O7."2Sk ° GN 2813 12 ^2801 2806 ' , '2398 1.2406 2802 2803 TJ 2735A U4912 U4902 M+4-22-27 79 77^ Mi 3-24 2750 2743 U4746 69 V U4740 U4758 _ __________ •: 2738 2737 U4780 • U4773 о ( о M+3-23-32 2 61 2™>2744 2752^ .1 275 Г '°2/45 • 2749 ^04722 U4542 L | ' 2622 №№ о GG . +23 M+3-23-22 ~ ®FZ [4+4-21-25 о ° U4669 'M+3-23-19 °U4596 M+3-23-13 0 26732672 2677^^ -------------T U4925 ‘ 83 • л 2797 о 1/4761 U4729 tW,c 09h20m 09h16m 09hl2m 09h08m 09h04,n -M+3-23-21 OghoO111 08h56m 08h52m Open Star Clusters and Asterisms Globular Star Clusters to \( rile to scale < 5' Planetary Nebulae Bright & Dark Nebulae to scale □ >5 to scale Galaxies >30" 30" 10’ 10" 5" <5" 10*-5 о о 1 5-2’ 2-1 < major axis Ase lus Borealis < 437 XX U4504 40 38 BT • 2624 264\ Л, ® 4 • 2647 2637 ,2.625 ’ . 41 E 2632 M 44 U4526 ;л- * • • Beehive (Ргаея ^409. -- л . e Asellus Austraji^47 0 +19° М+3-22-20 +1 08h36r 08h48m Galaxy Cluster to scale 08h36m to 10h04m +30° to+17° CMC LEO, LMI И/ll1 T/fian / forty fryifYipnil/ Will Rentaklm
75 08h44m +30° 08h40m 08h36m K/50-/4 +27° +26° +24° L_ М+5-21-10 2619 4692' ъ 2623 M+4 -21-7 2621 2622 2620 2628 о М+4-2 0-69 ^6М +29° +28° U , U4542 +25° +23° +22° Asellus Borealis ♦ 43у +21° UV +20° M+4 -21-13 о XX U4504 0@ лп39 • .• 2643* '42* 18ВТ -2647 о •<> ' 2637 , 41 ЕТ* 04526.л- • 2624 4 • •2625 2632 M 44 + 19° _ ‘•о ТХ , U4532 0839+187 ® /•2392 Asellus ’47 X JA8— ustralis# i-.0-.-" + 18° !- — _ 08h32m 08h28m 08h24m 08h20m 08hl 6m 08h08m 08h04m GEMINI 15 BM @ M+5-19-37 M+5-19-38 С М+5-20-3 08h12m C148-115 CANCER 2604 C149-19 +29° 2608 • U4425 +28° C150-5 18/ 114341^ 2607 ^>23 0; 2540 U4464 1.492 • +26° О .485 .486 0 о U4300 U4364 С149-50 о ' С149-34 ___ •____4^4340 2576 * о U4346 М+5-20-7 2592 2594 ' A 3C200 o U4395 22 0’-^ а 1.2361 1.2365 M+5-20-1'1 08h00m - +30° М+5-19-30 1.508 U4373 0 1.2267 U4301 oRX C148-117 1.2219 1.2217 О М+5-19-33 \ +27° 32 Ъ2е . L509^ 2599 ©301)' ®28СХ • .. 1.2382 • . q2598 • • • 331] • FS ♦ 0 • M+3-22-16 • ,35 0 M+3-22-18 12.5' b U4457 U4414 ° °U4400 ^-2595 о 2582 1.2373 _ V^Beehive'(Praesepe) °U 126' 127' М+3-22-20 + 17° L LCANC£R I 08844П1 ~ ~08h40" 08h36m 3C202 лЗС201 @31 0 U4433 С* 08h32m о 2575 19X о U4304 о 1.2239 О 2554 1.2248 iU4299 О CJU4406 U4416 1.2363 о •о 2581 0 . о2^ °U4444 2?96 08h28m •^La Stellar Magnitudes (V) 0 5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 U4375 О о 2577 1.2341 ‘ .° L2338 08h24m О М+4-20-34 ^65 2557 . 1.2293 V U4332 2562 ( 2563 о0 3C197 U4308 U4329 <>1.2253 2О5.45 ^^2556— ° 2553 ° ZU4324 у ° 1.496 13 4 1|/ф • л2535 ®2536 U4257 о 1-493 3C192 ©9 BL 10Ц 2 0) •: о • 1.482 4 • : | -"рл—° +25° - hu : 2498 +24° 2512 о М+4-19-17 +23° 2503 +11° Cl 18-40 й +21° • 0 2558 119' 121 123' +19° • 20 d1 +18° C89-16 -о--------- М+3-22-8 - -4 U4386 2570 э О 1.2340 U42070 1.2329 .. °2572 2569 . U4344 ^119-51 Cancer Cluster ♦ - 2522 08h20m 08h16m 08h12m 08h00m 08h08m 08h04m U4269 9 • VV Double or Multiple Stars Individudl members are plotted if separation exceeds 60 120' M+3-21-15' 118° GEM +20° U4286 L/4245 о 2530 Variable Stars О ® (•) ® ® (•)(•) о Amplitude Amplitude Amplitude Amplitude 1.0 maq. or less 2.0 mag. 3.0 mag. 4.0 mag. n Nova Q Quasar A Radio Source X X-Ray Source Copyright 1987-2001 Willmonn-Bell, Inc.
। Of h00m 07h56m 07h52m 07h48m 07h44m 07h40m 07h36m 07h32m 07h28rr*_ 07h24m 07h20n 1 07h16 (J J777I +30° +29° .30' • GEMINI 1 • • • • • Д602; • * - -z U4042 • • • _ C148-19 cl .1 ♦ =, ( • J3995 M+5-18-26 2147-51 • C147-48 о о • • • • • • < 2371-72 • • • •oC147-i; M+5-18-7 u • oV33y +29° +28° +27° J 0 0 +26° r ' r 2 CO • <4 +25° 1 +24° к ♦ • • • • • • • • ♦ • • • • U403 • M+5 C148-6 ° • • о 0 78 p 19-4 Лк ?5(5- • • 0 M+5- 8- • M+5-18-25 ’ 24 • 0 • • • • • 64 • • • • • . 53 1 +28° • - +27° • • 4610 Ль 2490 • • . /.479 C148-39 • Pollux • 2450 • • • • • ♦ • •_ : • -0 • r« * zfL0 03876 65 b • 601 «59 M+5-18-1 • • • M+5-17-19q • • —-•- ~~~~~ 2492 1/4705 .485 /.486 • • 0 o >83 Ф 1.480 9 о • • • • a 0 2449 • • 4 " * • • • • 691) ♦ • о U3874 • • ..C • • • . . . M+ •117-41 • 4-18-9 • • • oV340 • • • J +26° -•- о I • ° • • 0 1.482 2487&o 2486 ♦ Cl 18-21 • • • — «> • • 76e • . • • • • • ° 2 • • • 405 ♦ ♦ • ’ _ V341 - • • о • 57 • ГЯ-г • • RK Cl I/-0 • 3808 Л — +25 • 1 гтт-2498 7- • 4 • • U4099 * C118-18 . о • • • • • • • СП8-5 * 1 0 ’ • 77 K > • • • • • • • • NQ О • • г о ^03 2398 * #д3’ 869 C182‘ • • • • • _ • — • +2 • 4° ЕЭ 23° +22° +21° • - +20° • • -j +19' 2480 2481® .M+4-19-17 J • • • • • • о U4054 • oT о C118-14 • * 0 . • . Cl 18-3 • • J4031 • • Cl 17-6. °S * U396 • ♦ ? < • • • • • 0 • • • • qU3911' • • 2370 c> • 2376 о • • о ° м с • • 58’ • .4-I87 • . 4- —+ +23° 2503 +22° r • +21° r 1 • • 84 • U • 82 • • • • • • • • • • • • • • . • ° U3932 • • • • '-омз' • Cl 17-3. из -© • U3806 ° о • • 1 U3824 •. 827 a 2365. ^3803' _ I -— — 109c —#- \A/;KAt 55 0 • • ♦ • о ♦ © • M+4-19-3 • • • • • »" ♦ • • • 114° " [diptlC • 2420 • i- • • • • • • • 1 " no6’ • • ГТ“ f. 1.2186 1.2188 . • • 1 • » • • • ♦ • M+4-/9-7 ♦ | 1 0 • • • 6°\. • • • • • ♦ • 79 « • Л • • • • • • • • — • • • • • • 2392 . ’ ’ 0 ,• U382 M+3-19-18 0 skimo Nebula • 3 U3862 ♦ ..•61 • ♦ • • • • 56 • • • • +20° » +19° - • • ( +18° - • 3 • • • • • 85 . • ♦ • • • • • • U3939 • • • ♦ • • 0 U390 • • • 3 » I ’ м+3-19-13 M+3-19-14 • U384C e си3842 ^ • .11 • о ° ' • • • • 34140 ’ . 0 • • • • • 0 . U4044 • ♦ • • • 81 g • • — — • • • • ° C87-25 • • U3920 • •’[ 2411 • 5 • • 2407 * о 2406 йМ+3-19-2 -© 0 • < U3823 • • • • •• • 1Э0ЛС • • •» • • • ’ GEMI ——•— - • — +11 • 4 07h16' M+3-21-2 • ♦ • • CANCER • • • • • • • • • • •» • • • • • • • • • • .1 74 P * . 24 №. s ® 0735+178 • • , M+3-20-7 118 • • • ♦ • *c C87-4 • • J» - • • • • 1—J1 —.-F— • • . u3820 3C1 —{ л n л m П UjoUj • • Г 76 7b?0m +170’1- 08h0( — —♦ u .• лчЬээт 07h?8m U/"^ )m 07h56m 07h52m 07h48m 07h44m 07h40m 07 36 07 Wil Tinon I Barry' Rappoport / Wil) Remaklus
76 + +2 07h24m -30° • • • *oCb ♦ S M+5 29° — — _ • • 8° • 07h20m • • из 17-13 -18-7 e -V339 • • • • • • • 07h16m L o' 777 '1 • • 461л 3728 0 —r- — —«. «_ • U3692 • • 6 из 731 • • • О • * U3702 • • • • • • • 7h08m 07 ) J • • u. • аМ+5-h • • • • ♦ h04m 07h U3631 . < ♦ •9 •• 1649 * • i 7-10 00m 06hi 1 •_ • • • • ♦ • • • • • • • >6m 06h5 • • • • • • U3571 • ♦ • • • 2m 06h48 • M+5-16-7 I • • • • • 03552o * • • m 06h44n • 13536O>\. C145-6q ‘ • 28 • • O3518:> ♦ • 0 06h40IT —I +- GEMINI Al • • • • • • + • 1 1 • • 1 • *1 • ♦ 25 * : 0° JR 29° 54 28° • 601 +22 • 59 5 M+5-17-19 • • • 3® J U3745 ♦ • :i46-40 • • • — —« • • : 233i • M+5^17-7 ’ • ♦ ♦ • • • • • I M+5-17-2 0 . • • &• * M+5 Ь U3585 о U358 • • 1/3573 -16-10 • 4 e • • ♦ • • • • • +27° +26 • M+4-18-9 . • © V34( • e. ♦ ) • • • • • • 47 • • * 1.2180 • • • • • • • • s _• _ • • • • • Wo *39 • • • • ♦ • • 0 Cl 15-14 • • •2266 • ♦ • • • * +26° +25° • 0 a 17-6 • 808 49 • <=> U3726 • • • • • • U3674 ’ ’ , 4 .. / •A3C172 • — rr o< • • • -• • • M+ •37 ее Cl 16-3 • M+4-16-2 • M+4-16- 4-16-5 M+4-16 03555 ®QU • • • A- U35 31.-, -3 • Mebsuta • • • • QR • 0 ►-27E ’ +25° +24° • BM • • • ♦ • • • ♦ ” ——— — <52 ♦ • 0 oV338 48 . ♦ • • • • • • 42(0 • • ♦ • • .. U3599 • • • • ♦ • ♦ • • • • • • • • •+24° /V <a . +23° • 1+4-18-14 ' ° ° M+4-1 ° kA 1 • M+ • • • CO • • • ’ 8-7 . 4-18-5 2357 • • • U3770 . *U3753 ♦ о U3751 • • & ♦ • • U3676 ф M+4 • • • ♦ • -17-6 • • ♦ • • • • • • e • • ° U3594 e • 0 M+ • • 1-17-1 • * e • • • • • • ♦ 3C165 • л * joo;\ +23° Cl 17-3; U382 +22° к J- +21° - о U3806 ° • U3824 • 7* 2365 ... - - - -<7_ • 109° -Л* Wasat | < 1.2186 8 1.2188 ——- 108\_ ЙМз’’ 6 5 • • • . ° M+4- i or....... "'Ecliptic < <•> • ♦ • '7-10 [06’ • Cl 16-24 . • .7 • • • • • • ’ <> R . 44 • "°iw~ ,0*° 03 • • • • 104° • • • 652 .©V335 • • • • • 10Л • • • • • • • • • • • • • -."'/"То, • °C11 • • • • 170 ' • • 6-2 • • • • 36d • • • • h— 0“ 0,s ♦ U35 34 • о • • • . л 3C166 • • ♦ • • • e •DI — P19 • • - +22° 2.5+7.2 -1 +21° • +20° — • • >56 • • • • • • • • • • • 2342<l' . 2341 • • • ж • • • . < 43; • • Mekbuda • • • • i • U3611 • • • • • • • • • • • ♦ ’• W55J 03553 /oQS • • • • • • • "AD • • • ♦ • • 0 1 • - +20° • +19° L— • • • • • < • 4 • • • ' 1.2181 ’ • • 1 . • • • • 0 U3678 • • ♦ U3639 M+3-1 • • • • 8-5 • • • • 035S7o; • • • • • • • • • e • • • • • • • e • • • — +19° и • ♦ +18° 3823 ’ ‘ • • • ♦ ♦ • 4 • • • • ♦ • • 2339° • • • • • • • ♦ M+3-18-9 • • • • * M+3-18-7 •• o C85-23 0 M+3-18-6 • • • • • • ♦ • • • • • 2304 • • • • e e e • • • • < • • e e • • • • • — +18° GE • I +17° LJ_ 07h24m **U3805 MINI • 1 07h20m • • • • • [_u 07h16m ♦ • • • 3766 t> — 07h12 • • ♦ • m 07hoe • . U3658 ♦ • !m 07h0 NR® • • U3635 ° 4m 07h( . ® • • • QY . • 0 qz ; • • • )0m 06h 0 • 56m* 06 •• 0 • • h52m 0( ♦ • • • • ^48* 0 • • • • 26 ’ • • • • 6h44m • ♦ • +17° 06h40m Copyrights 1987-2001 Wittmann-Bell. 1гк
06h40m +30° 06h00m 06h04m 06h08m 06h20m 06h24m 06h36m 06h32m 06h28m +29°. AURIGA GEMINI +27° +26° +24° +23°. +2Г • . S4X' +20° +19° +18° m <25 +28° +28° +26° +27° +21° 40 DW ' © Cr89 P 89.8+7.7 • 92 .444 3C757 • U3503 RZ ®TV U3489 uo 8e 23 2163 VI391 20 ®VI155 GEMINI VI387 ORION L • 05h56m 06h00m 06h04m 06h08m 06h12m 06h16m 06h20m 06h24m 06h36m PV ----? +24° +22° +29° 06*32" 2234 06*28" „ . - 90 • 2129 ® .• +17° 06h40m . 54 U3447 о U3450 .<115-6 3C160 • 44 К < • • • • • • • _j. J- ®V394 • • • • • V395 • P183.8+5.5 • eV451 • • . °V450 • • • • • • • • • • • • •• • • • • • • • ' ► ♦ P184.8 • • 3(154 Q ^4.4 • • . TU • ’’ -AA -•— — • • • • - -• • • • < . AURIGA TAURUS 139 . P184.6+0.6 +25° I- 3C162’ 10 11 LU®' ’ © LT 9PX 94° 99 WYg Ecliptic 13 u +22° I—• Pl 92.5+7.2 V963 • 22 18 V Bo 1 2218 . OU Pl 94.2+2.5 2168 M 35 1.2156 2158 1.2157 3PU. Open Star Clusters and Asterisms Globular Star Clusters Planetary Nebulae Bright & Dark Nebulae to scale □ to scale to scale < S' >30" 30’-10" 10"-5" <5" IO* -S' © 6BU Propus 7П . 2175.1 3C152 8227 Skiff 10619.3+1832 1.2162 Sh2-257 Galaxies lo scale 2 1 < major axis RW^1_.-TAURUS- +23° •4 •l40 ... - -o- - BQ ORION GEMINI Bas 11b 64 V1385 +19 +18° “,yc'u““ 05h56m to 07h24m +30° to scale GEM ORI, AUR, TAU W/l firiori f Burry Ruppapurt / Will Remuklui
06h04m + 30° 06h00m 05h56m 05h52m 05h48m 05h44m 05h40m 05h36m Cz23 AURIGA TAURUS * SV Pl 81.5+0.9-& V781 2129$ GEMINI ORION 64 VI385 .0 V593°* ° /Л Pl 84.6+0.6 4/ ' <#/ ® ------ 140 BQ°' Bas 1 lb Cz24 • V438 о ©V433 о V1163 AB Sh2-240 Simeis 147 „ЕТ • •V725 V1167 / ° 4/ • * 88° . - b------------- Ecliptic Be 72 1996 Be 21 PI 84.0-2.1 ®V1165 * 2026 •127. U3341 05h28m 05h32m DoDz 4 • • • ♦ • • - • 0 V362 1896 P178.3-2.5 • Alnath • • • ilTp • • • ♦ • • ; DoD • • • z3 • ♦ • • • • <111 • Д I 3CI39.2 • SN 1054 Crab Nebuo 1952 M 1 (Taurus A) 119 CE 120 (V960) о V1160 ______82° VI028 I14o 05h24m Be 19 •22 05h20m 30° • • + 29° • • • • J f280 • • +27° • +26° • ♦ • +25° • ♦ • - +24° 8Г - +23° • • 109 n • +22 ♦ • +2Г • • • • ♦ +20° V115 9® U3363 111 (V1119) ORION TAURUS 117® • 06h04m 06h00m 05h56m 05h52m 05h48m 05h44m 05h40m 05h36m 05h32m 05h28m 05h24m 05h20m Stellar Magnitudes (V) • • T ,s » « « » „ aftdbnghtet u--> l,u Double or Multiple Stars -ф- • ♦ * Individual members are plotted if separation exceeds 60r Variable Stars • @ ® ® (•) © © ®®° Amplitude Amplitude Amplitude ^ude 1.0 maq. or less 2.0 maq. 3 0 м Nova Q Quasar A Radio Source X X-Ray Source Copyright C 1987-2001 Willmann-Belt. Inc.
Open Star Clusters and Asterisms О О О to scale < S' Globular Star Clusters Ф Ф Ф to scale < S' Planetary Nebulae -0- < >30’ 30" 10" 10" 5" <5" Bright & Dark Nebulae С?<'у □ O :; to scale 10"-S' <5‘ Ge A >5 to scale laxies О о о 5*-2* 2"-Г <1* major axis Galaxy Cluster ; xi to scale 04h36m to 06h04m +30° to+17° TAU AUR, 0RI, GEM Wil Tinon / Bony Rappoport / Will Renwkhn
04h40m 04h36m 04h32m 04h04m 04h28m 04h08m 04h24m 04h12m 04h20m 04h16m B23 - • TAURUS B24 42 у +29° 87 8209: kRW • +28° BIO +28° Do 14 U2964 +27° B207 M+4-10-15 +26° +26 U2931 1508* +25° 8208 +25' VI135 M+4-10-17 36 +24‘ VI136 M+440-24 +22° +21° +2Г M+3-11-: U3135 +20° +20‘ + 19° +19* + 18° !- U2988 0 VII37 3C108 •co 0 . U2958 A 3C123 U2989 о о 0 U2976 Taurus Dark Glo^id 822 , +22° +27° +23" +29' fi220 1.2087 U2928 0 M+4-10-4 1497 og ♦ -Г -U29274 B2 19 V833 819 8216 <& 59 X 8215 818 oV1139 * 72 691) 65 K’ 39 70° 69a 65е V834 50(0 4-: 74 e 68 83 04h00m 04h04m 04h08m Double or Multiple Stars (.opynghtV Г 9*7-200» W>Hmunn Bell. Me A Amplitude 1.0 mag. or less Amplitude 2.0 mag Individual members are plotted if separation exceeds 60“ o.o and bright^ Amplitude 3.0 mag. ®V1142 6S 7.0 7.5 8.0 8.5 9 0 9.S 9.7 8218 B217 95 +24* 04644m +30° • • • V11400 B214 V987 +23° u VI081 + 17° - 04644m TAURUS J‘W/29 04h40m P174.2-14.6 © HU U3099 1615 ‘. V1149 ’ ®SZ 04h36m 04h32m Stellar Magnitudes (V) B18 Vtu J J °DF e • • * к Ced 34 04h28m 62 ♦ 67 K? 68° • 64 82 04h00m - • +30' 41 GS 1.359 о B211 52 ф 8213 <=> 1539 44 IM p U3009 8212 M+4-10-28 ^8210 . V1134 о . О ’ U2949 C'r—— 67° tchptic © ® 56 (V724) • 51 53 Hind's Variable Nebula • (Struve's Lost Nebula) □ 1554/55 . 3C” 61 6’ H у a d e 5 0 U2968 ______1--- 04h24m 04h20m 04h16m 04h12m Variable Stars 37 JOH57 * U2942 ° M+4-10-9 M+4-10-11' M+4-/0-I2 M+4-10-14 63е 1.358 Nova Quasar Radio Source X-Ray Source
03h20m 03h24m 03h28m 03h32m 03h52m 03h36m 03h48m 03h44m 03h40m ARIES vdB16 +29 +28° +27°- +26° +25° +24° +23° +22° +21° +26° +19“ +24° +20° +27° +25° +29° +28° a 62 V837 .1995 о AR о AT t64 2 SY- A450 66 J2840 32 65 • 13 VI124 VI123 TAURUS 1 ARIES ‘ U2684 • V471 03h20m 03h24m 03h28m 03h32m 04h00m 03h36m 03h56m 03h40m 03h52m 03h48m 03h44m 1/2797 • 9 18. „21 1432 +22° +19° +18° 04h00m 03h56m +30’ --- TAURUS 03h16m —, +30° 1.353 28 BU <• I oV624 \)16 vd820 M45 Pleiades •• 25 П • 26 S 1.349 ЪМ+3-11-3 C466-3 к 59 60S 33 (V817) © . BL 60° 1.355 Pl 71.3-25.8 . U2892 - Tempel's Nebula (Merope Nebula) 1435 • M+3-10-1 О AS 61 T 63 +23 C465-3 c. U2809 o- 57° M+3-10-2 '* U2716 d 1.1977 +20° s XX EclWc +17° 03h16m Open Star Clusters and Asterisms to scale < 5' Globular Star Clusters Ф ф e to scale < 5' Planetary Nebulae Bright & Dark Nebulae ч> 4 / П □ □ : >30 30"-10" 10 -5 <5“ to scale 10 -5' <5' & >5' to scale daxies О О о 5'-2’ 2'-Г <Г major axis c~ 03h16m to 04h44m +30° to +17° TAU ARI VW rinwi / Hut,У / Writ Кепюккл
79 03h24m +30° 03h20m 03h16m 03h12m 03h08m 03h04m 02h48m 02h44m ARIES . +29” +29 1056 +28° +28 +27” +26’ +25’ 64 +24° m 02151 39 RS • 35 56 SX 33 +27 +26 60 • wz vz® 0 AR 02457 +23 +23 02530 +22 32 \ AK +21 +20 34 Ц + 19° +19 45 RZ + 18° 46 р 02716 so* • 44 36 • 51# 49 • M+5-7-50 Lsl_____•_ 02486 1.1854 0 <5 1.1841 02563 0 ‘М+3-8-2/ 02296 о 1° M+3-7-42^ 02303 02286 02327 1030 0+18 M+4-8-4 ^M+4-8-1 02442 1156 1.248 о 0 M+3-7-40 1036 0 1.1832 ___s________ 1054 M+3-7-47 °' 02290 M+4-7-26 55__ • • • • • 02497^^ • • -2 # JU UZ' • • • 'DZ'" ♦ • • • • 02h40m --- +3C • 62 • 59 +22° • M+4-8- • /2 * • +21° • 65 +20° J- 1 61T • ♦ 63 • * • T • I • • • • • • ♦ • • r. .. ^02570 1 • ♦ • • • • •—. >576 02553 •о 1.1890 54* М+3-9-5 о ЭХХ ° 02684 о U2498 ДЗС79 <8° 03h20m 03h16m O3h12m • 53 М+3-9-/ U2506 U2272 1.1861 +25 48 £ М+3-8-4/ 50 i /° 03h24m ARIES ' 03h08m 03h04m 03h00m M+4-8-3 ‘AP 02267 • 47 0 02424 42Л о ° AM М+3-8-11 DoDz 1 +24 02h56m 02h52m 02h48m 02h44m 02h40m Stellar Magnitudes (V) фффффффо****** 05 1.0 1.5 20 25 50 3 5 40 4.5 50 5.5 60 6.5 7.0 7.5 8.0 8.5 90 9.5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60“ Variable Stars • ® ® ® (•) ® ® ® ® о Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag 3.0 mag. 4 0 mag м Nova Q Quasar A Radio Source X X-Ray Source Copyright Г) 1987-2001 Witlmonn-MI. Inc
02h40m +30° r— 79 02h24m 02h20m +29° +28° 33 U2122 \U2151 U2134 +27° ----7 +26° +25° Q2^6mC505-17 02h32^ 0 972 M+4-7-15 С» M+4-7-19 M+4-7-17O o U2082 30 • M+4-7-13 +24° f—- 02079 C1\ U2104 о +23° +22° МК +21° I •o 992 +20° 0 +19° +18’ 02h28m о U2053 12 953 U2017o 962 • о 02h16m 02h12m U1696 ° t>U1690 02h08m 02h04m 02h00m AJ1792 . -I-----®- U1971 о TRIANGULUM 1.227 T 1226 U1596 uU1591 i I e о I. Ш590 816 819°° 01 h56m - n +30° +29° AD 4C+28.05 10 • 1.1753 ARIES о M+4-5-2 7 M+4-5-36 TRIANGULUM M+4-5-47 0 784 0 • 865 о : • C482-55 J.188 * 1.187 U1533 I . 0 . 1Л549 • M+4-5-46 807^~.' .^805 . ° C504-2 +28° 855 +27° +26° 20 6 14 . U1648 U1739 * M+4-6-1 о 765 M+4-6-2 +24° U1752 »901 J900 U'462 * ^01808 м+4-6-15^ °AE M+4-5-31 s 1.190^ 1.189 '77(> •'9^ |®7RR M+4-6-22 o • 0 0 M+4-6-19 U1812 ',7“‘OCU,^VI,S1 • C482-35 4 U1561 . c U1478 OU1551 . °U1833 ° C504-69 0 • 1.221 4C+27.08 ‘ U/565 о o. 780 U1899 »n U1892 M+4-6-32 oU1885 928 . 9^915 о 01844 U1921 ° i/ U1881 • . U1939o . , 7 ? o °. о M+4-6-49 M+4-7-3 M+4-7-2 -j-------^891 U2025 о J1218 • U1860 M+4-6-26 W+tAZ U1955 AOH ° M+4-7-6 U19 70 M+4-6-42 „ I M+4-6-36 a___ U1917 M+4-6-29 M+4-6-16 U1706 •• ©AC +25° M+4-7-5 o ч M+4-6-28 M+4-6-43 о 984 U2020 •' . M+4-6-61^ 1.1803 O'(J1938 . M+4-6-60-^ 2> | о M+4-6-44 О 1.1806 1.1809 ° , ° • /. 1807 M+4-6-31 ® AF M+4-6-11* .M+4-6-10 Hamal 13a 12 К oAA +23° U2028 о 0 , M+4-7-8 00 M+3-7-24 M+3-7-26 ' • о U1871 '(J1733 17 П M+3-6-40 0 о AB Ul 547 о U1490 +22° * 0 976 U2012 . U2064. M+3-7-36Oy M+3-7-31' . M+3-7-32 ° . о I . 1.235 0 U2031 1036 &U2I40 U2140A +17° ।— 02h40m '° M+3-7-19 U1965 M+3-7-13 ‘ ^924 ^932 . 938 о 26 M+3-6-50 C462-23 о = 1/1999 о U1652 U1514 0 ^01485 о9 C461-14 C461-15 - +2Г Sheratan fl 722 935 1.180113 v M+3-7-20 • 22 e •23 • ®AD 1030 M+3-7-5 ARIES 0 918 M+3-7-23, C461-70 7Г >27 M+3-7-6 02h32m 02h28m 02h24m • 02h20m +20° 0 M+3-6-37 U1560 J U1433 ©15 о M+3-6-3 M+3-6-44 M+3-6-41 U1519 oU1518 172 о U1445 770 +19° OU1731 0 M+3-6-32 M+3-6-49 ----------- M+3-6-47 о M+3-6-42 о UY .817 02h16m 02h12m 02h08m U1546 0 о 794 о M+3-6-17 0^ M+3-6-18 U1495 81 1.1748 - U1531 о ’ о 01432 02h04m 02h00m □ 10 - 5' Globular Star Clusters I Planetary Nebulae Galaxies to scale to scale i Open Star clusters I and Asterisms >30* 30".io* IO".5" <5- Bright & Dark Nebulae to scale io scalp У-2' 2-.r < major axis Calaxy Cluster ------- 01 56" to 03h24m +30° to scale ARI TRI +18° 01h56m
80 02h04m +30° (-- 01 h20m --- +30 02h00m 01h56m 01 h52m 01 h24m 01h44m 01 h28m 01 h40m 01 h32m 01 h36m PISCES M+5-4-56 +29° +29 3C42 +28' X« 90 • +27° о 765 697 о /.167 ° VV 1.1764 0 ARIES; • С482-55 ° 805 . О °\С504-2 М4 oU1233 Г- U1228 о. 780 4С+28.05 • "1.1753 01h48m +28° 1.1672 о 1.96 U1154 M+5-5-1 © +27’ +26' U1230 +25 4С+24.02 ® 7 RR о АА 1.1742 оАЕ RW- ° RX 575 606 С467-75 ’ U899 ЗС47 . С459-66 722 107 0 U1375 U1433 А179 М+3-4-45 А225 U1025 U1243 ©97VX . U1104 1.1701 М+3-5-37 • 92 с U1219 а 1.1711 U 093 о • 794 о 719 1/7077 1.115 U1032 о; U1531 о U1197 U1432 U1396 81 1.1748 U1514 о LU1560 C.U903 ° U1372 о 711 М+4-5-31 ’с /. 190 °о I. /59 Г 776 М+3-4-21 • . 5 6.0 М+3-6-18 О U1495 U1519 о. • oU1518 U1099 о U1098 . о U1490 ’ С461-14 о °* ^!485 ’ U1o84U1369 * °11786 Ш399 а Ш329 о U1020 • М+3-4-3 772 U1445 ^770 U1546 о М+3-6-17 ° С460-18 1 U1359 0 r — » °шзн 2a • • М+4-5-27 684 о 0 670 М+4-5-3 о TRIANGULUM “• М+5+-33 ’ ° *4 • 91 М+5-4-49 . м+5.4.31 М+4-5-36 U1533 1.1731 О' гСг21 <M72 О 1727 М+4-5-7 • о -.'1.188 М+4-5-46 М+4-5-47 U1462 ъ о U1451 М+4-5-70 656 1/1073 +25° — +24° +23° +22° +21° +20° +19° + 18° и ^Ш453 IU1479 ш *С482-35 и\561 . о U1478 ОШ551 М+4-5-6 о М+4-5-7 s М+4-5-8 CZ U900 *695 +24' 3C43 6 +23‘ 0/547 I 0 о М+3-6-3 17° — 02h04^ = zz 02h00m 01h56m 694 678 ---о---сто— 680 697 1.1725 1.163 +22‘ +2Г U1265 0- Mesartim о U1324 01h52m Stellar Magnitudes (V) SV 109 +20’ ARIES 01 h48m PISCES •М+3-5-13 01h44m 01 h40m u » » ... » «♦»»“ “ “ ” ” 11M ” Copyright C 1987-2001 Wamann-BeH, Inc. М+3-4-47 \ М+3-4-46 М+3-4-37 L^94 Г • 93 р Д795 U851o +19’ М+3-5-9 М+3'5'] ‘ U1173 о U1119 01 h36m 01 h32m 01h28m 4 01 h24m Double or Multiple Stars Individual members ate plotted if separation exceeds 60' Amplitude 1.0 mag. or less Variable Stars Q A Amplitude Amplitude Amplitude 2.0 mag. 3-0 mag 4 0 mag. X о С459-40 ’ * U904 С459-29 +18’ U883 I +1 01h20m Nova Quasar Radio Source X-Ray Source
80 00h40m 00h56m 01h00m 01 h04rn 01 hl 6m U524 M+5-3-32 °U542t U540 +29° 68 h 911 +28° 901) +26° ®CR M+3-3-16 01h00m 0 U628 U556 +28” +25” +27” +29° +27’ » C459-10 81 \|/J 00h48m 243 02h44n1* 01h20m +30’ 1.1672 О /.96 00h36+30” 83 т 01h08m 74 U696 10654 00h52m _________ _____________ ЛБ 0 I О PISCES KS .M-S-2'47 , 0529 ° ' p-M+5-2-45 (43 1.46 +25” 36 0425 +23° 0109+224 +22” 84 X +21” 0723 +20” 251 +19” U617 +18’ '4154 «459 0751 i 00h36m 00h40m PISCES 00h44m 4158 00h52m 01h04m 01h08m 01h12m 01 h16m M+3-4-21 +18” +22’ +24” 0(/845 • +19’ +20” +21’ °C459-29 [W-8’'A71 30 £ о ‘ 0371 64 •00h48m M+3-4-15 0 U851 +26’ «10360 „ 0 U367 о О л U398 17’ --- 01h20m M+4-3-42 ' M+4-3-43 M+4-3-39 0 M+4-3-40 0643 0 U629 U636O «354 65 0 C5C • 1-18 U501 260 ° 1.1584 258 252 •M м+4-3-21* 67 0_____—IL. ° 326 3C28 CNo LM69 M+4-3-2O0 0052+251 M+4-3-16 'A104 U612 о M+4-3-26 ° I 304 U591 cp M+4-3-27 U605 • • M+4-3- M+4-3-8 -0506^ i- M+4-2-39 0 M+4-2-53 34; 1.1585л 11 79 \|/2 M+4-2-46 0411^ Л+4-245 0214 229 228 M+4-2-50 U510 ANDROMEDA • о • • 1.1596 ’ • • • 1 • • • ( — - • • — М+3-3-6 • 161 • • • . M+3-3- оСМ 9 • * 1 • - М+3-3-1 о — •-— те. г • 59 °U477 66 O 11616 00h56m C4 79-54 M+4-2-43 1691162 1.1559 160 +23 475 54 4C+18.02 0393 M+3-2-19 О PISCES Open Star Clusters and Asterisms 0 0 0 to scale < 5' Globular Star Clusters ф ф Ф to scale < 5’ Planetary Nebulae -С1)- -ф- -ф- i ’ >30" 30"-10" 10"-5" <5’ Bright & Dark Nebulae to scale 10'-5‘ <5' Ga >5' to scale laxies 0 0 0 5' 2' 2'1' <V major axis Galaxy Cluster to scale 00h36m to 02h04m +30° to+17° PSC ARI, AND, TRI
00h40m 00h36m 00h32m 00h28m 00h24m 00h20m 00h16m 00h12m 87*00h08m , 00h04m 00h00m + lo iГ——।I-----s ------------------------- --- ----------------------------------------- 4.1 + 17 ‘ PISCES U393 0 о M+3-2-19 о • • • • e 9 47TV •/ • . A43 Г" Ф- • 1 • • • • • • 57 0) • о 1.4 ‘ U122 • • • U46 о • ^U31 • • =1 U12893 HO +1 7 +16 • • • • • • • <-49 • • ► 48 о . U250 • • 700 40 • < 1 • *39 • U148 D • • • . NP • • • • S4C+15.01 • 0 1.5378 •* • • 07814 +16* +15* Q +14' '•9 +13' +12' • • • +11° +10° +15° • • 53 AC U3 86 f_ Q_ • • О • 1/290 • • • 99 3C9Q — • • • • • • Algenib 88 0 14 • • • • и *5 1.5381 • 17 • M+2-1-14 о . +14° • eTW • T • о U233 ° • 43 • 01/226 • • — LN • • • • • • • • • 7800 • +13° U385 Л 3C16 • • • • • • ♦ L/305o • * Q 0026+129 о U249 42 • • 37* • M+2-1-31 0 • • • PEGASUS • о 1/99 • • • • 86 • • M+2-1-12^*!*2 7803- +12° M+2-2-22 c • • о 1.31 • 0 105 • • ♦ • • co -< о • 1 o. 0 U132 • • • • • • • •: • • < 7810 • > NN фа +11° • • < • • • M+2-2-/3 • * u< -♦ • '60 &M+2-2-10 • • ♦ • • • 63 о ‘ • • ♦ <34 • • • • 1.1526 ♦ + 10° J.35 • • 137 * о U287a • ♦ °CG О 95 • 1/191 ’ 0 1.7 • о . <S> • U151 о U81 • • • U23O • • ° M+2-1-16 • 4-09° • • 4J422 • о1-34. • • • • о • • • • • • ♦ • • • с • • • • 1/66 ♦ • • • - +09° • +08° - ^U418 • ° 180 • — • M+1-2’34 U3 • ( • oCH M+l-2-18 '! ' . J314 0 /.1557 • • • 41 d e ♦ 38 36 ♦ « о Ф35 UU • • • ♦ • о M+1-1-29 U52a ’ t 7838 a-7835 ^7834 *3 7837 •31 о M+1-1-13 0 о 32c • * • * U12890 Q. • +08° • • +07°.- M+1-2-36 о _,9!Lm+1-2-42 0 M+1-2- • • • • U335r. ^U331 26 • • • • 45* ’ • M+/-2-9 • /.73O _/J54£._ BX® • • oM+1-1-49 1/155 0 • • L/67 e • -♦ ♦ O7816 '7818 ’• — +07° U429 f U 1.1569 \ +06° I- 1.1568 ^1.1566 7/./565 476 • — O—• • • • oL/313 °M+1-2 ° U240 *U253 • M+1-2-4 -8 C409-1 < 4 • ° 75 • ♦ • • • G 0 36 • ' °7S2 °U36 • о • о U35 4 ®DR • • 7802 • • 28 0 B+06° +05° - 1.1564 • • • _ ° (7379 C409-37 о M+7-2-23 M+7-2-24 • 13 * “M+1-2-15 ’41 Ш ,9°O°'38 M+1-2- CD- 14 • • • • ° U143 • • • 0 U27 0002+051 * Q ° ?82\ 0 7825 °U3 • о M+1-1-16 • 7820 PISCES 3] •_ +05° 00h40m 00h36m 00h32m 00h28m 00h24m 00h20m 00h16m 00h12m 00h08m 00h04m 00h00m Stellar Magnitudes (V) • •••••••••••• alx,™,„ o.S 1.0 1.5 2.0 2 5 30 3.5 40 4 5 5.0 5.5 6.0 6 5 7.0 7.5 8 0 8.5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60’ Variable Stars • ® ® ® ® (•) ® ® @®0 Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4 0 mag и Nova Q Quasar A Radio Source X X-Ray Source Copyright C 1987-2001 WiHmann-BeH. Inc
00h00m 23h56m 23h52m 23h48m 23h44m 23h40m 23h36m 23h32m 23h28m 23h24n .100 Л r- ——г i 23h20n 1 + 8- 1 8° 17° 16° И 5° +14° +13° 26 +12° & • . +10° 9-65 - +09° T 1 О +17° * * +16° +15° < +14° В • • +13° • +12° r* +11° f +10° +09° • 0 +08°a if У +07° 1 +06° L PEGASUS • • U12843 M-t О . U12 1 -3-60-28 Mi • • 784 ’ • • • -3-60-23 • a 1)12710 • • 1)12707 • • • • 7681ъа M+3-59-60 о M+3-59-57 • /V • 1+3-59-47 1+3-59-46 . Г* • о . 7625 — + 0 1)12856 0 7792 • • 7772 • • • °V361 • • o M+3-60-25 • 76 • <74 М+3-б 7722 0 U12677 • • • 0-11 • 0 7703 • • • •— - U12582 7647 I'' M+8-59-53 ° A2589 ♦ • • / + •u • • • • • • ©V363 • ♦ • • M+2-60- • • • 17°- 1 • ♦ • \у . A2630 7691 • d7711 •' U 2 f- 1+2-59-42 OV351 7653 о * 601 * _ex— U12519 • • ^7800 * °u °M+2-60-25 • M+2 2822 • -60-18*- •, • • • • a • • • DIл 1)12653 ° о a О ‘ C432-2 U12613 о I Pegasus Dwt ' 7649 4 irf ! ° \ a / 7659 О A2593 • * 0 U12854 • * • "M+2-60-21 • • • • • I • A 4C+/3.< 0 112753 38 ’ . • • • • • • /644 7651 • • и ♦ • 12571 . 10- •> • • ♦ • • • • 1.1508 0 • ♦ • • • a 1)12687 •• • • • • 70 • • M+2-59-47 ° _• 7671 о о 7672 М+2-59-39 U12552 • M+2-59 7643 Qj • -• / • • • < — л A2675 1 о 1 / a 1.1513 й 1/727 • • 7774 • 93 M+2-60*13^ M+2-60-12 • • • • • ♦ • • ’1/72756 • • • ’ • • • • 0 7683 • • • 0 7641 7639 7638 0 . 7630 7794 о o. , * • • • U12871 • 860 82 ♦ • c, U12800 • • 7742o • • • • «77 DK * • • • • М+2-59-49:г • • • a • о 7 • • -DP • • • • • • • • • ® 80 HH о • 7743 . ../С+09.74 / / । • iA2657 • • • • о C407-5 • M+1-59-84 ^ • • U12581O - 7648 U12553„ . ° о M+1-5 U12561 UJ2S44- о • U12890 * • • • • 7780 cP M+ 7-< • U12818 50-44 s x* U12749 q M+1-60-23 2 • • • • 0 C407-1 • • • 7’ ч • • M+1-59-85 ° 7675 PEGASUS _ _._PISCES- ^ 7674 ’’ ' 1/72585 о M+1 -59-77 о 9 О Л+7-59-63 °34 S 762 763,S M+1-59-58— Pegasus I Cluster 7621 7679 ^7617 ^.+08° 2 r 7-59-5 9 - +07° • • ^Uo to 7778 ' 7787 7779 • C407-68 • 26 • • • *U12 • • • • 767 о о M+1-60- + 1-60-18 , M+V60-13 a 14 Y ОШ2688 • ‘ M+1 • M+1 -59-79 . -59-82 • • • • U1252 * • • 28(0 • • • M+1-6 • • • 0-39 о \ o M+ 1 1 0/757 ♦ 1-60-38 • • • • • » о M+1 -60- • 1 • • • • 100 • • • • • — +06° • +05° • • <?• ‘ • 7785 • • —S • 1 \ / A2665 • • • ♦ • • <-17l ^12717 • • • • • 0 U12689 * • • • • M+1 -5 9-78 О • • 7 _ 012548^012^ +051 L 00h0 gm 23h56m • 23h52m 23h48m 23h44m 23h40m 23h36m 23h32m 23h28m 23h24m 7 1Ц1 Wil Тюоп / Bany Rappapoa / WiU Remakkji
22h48m +18° 23h28m +18° г О M+3-59-57 23h24m 23h20m М+3-59+7 Г 23hl6m 23h12m 23h08m 0 + 16° +15° +14° M+3-59-46 PEGASUS • с . 7625 1.1472 23h04m 23h00m —— С453-38 22h56m 22h52m Ш2582/1Л л,гоп 7647i7A2589 М+3-59-53 Г M+3-59-30 U12495 P .M+3-59-29 U12350 ° О 74684 ^ 7468 O™4 М+2-59-42 oV351 7653^ Ш260Г /7649 /А2593 U12519 a U12506 M7H9122^ М+3-59-20 ° 7540- ,___7464,63 , 7448 7465^ 7461 • 7467 о 0 M+2-58-47 ° 7442 7659 о 7644 ' 7651 I 1/1257/ 0 U12552 70 7671 о 7643 о 7641 о М+2-59-39 +09° / 7674 7675 У 66 М+2-59-26 о I U12581O ° i U12561 Щ2544. -------о— М+1-59-63 + 10° Ul2585 о М+1-59-77 0 +08° < М+1 -59-82 о M+1-59-79 7639 7638 0 . 7630 +07° +06° 10 0 M+1-59-78 7580 —«— о 7593 +05° - 23h28m M+2-59-12 7509 7570 о 75594-к 7535 О 75598 ъ7536 7525 I ’ %7523 | о 7511 о 7505 ? • 7563 7515 о °7508 ЕОо . ™9о 7542 о 54 a Markab 1 •RW . 01.1461 U12258 ф °5Х • 0 М+3-58-7 ^HR л11к. © IM • • • • • • ^3C454.3 • М+2-58-33 ’ М+2-58-29 ♦ ♦ • 0 +16° + 15° °U12359 М+2-58-61 ° М+2-59-2 ъ I U12388* 7495 7500 Pal 13 0 7479 о Ul2308 7437 °V337 о М+2-58-46 4C+14.82 Q +14° M+2-58-48 M+2-58-50 ° о M+2-58-58 U12307 о 0 ' • U12281 М+2-58-39 74^4,3 7432 * . | ЗС455 U12253 VU12250 7405 о M+2-58-25 0 ’ 46 7610 114^1^05_ '^7616 7594 ~~~ Л I 7528 ° 'V347 ®4С+09.72 Г 7648 . I ‘ 7587 Ш2553 М+1:59-65\ ^°9 о • 7579 ±-7584 М+1-59-43 ° 7601 U12472 о 58 0 U12454 3C456 л 7529 V346 - U12407 аС406-13 57 GZ @55 .л*45 7631^ М+1-59-58 , . 7617/ 761/ U12522 45309 Q М+1 -59-59 С406-58 о Ш2548 2547 23h24m М+2-58-26 М+2-58-16 (о> о______________ 7?оо 7386 7382^7385 7389-^^-7383 7390- ' 7384 M.2-S1.2S +12° /_ 52 oR M+2-58-54 . M+1 -58-27 C405-33 M+1-58-32 0 M+2-58-42 о M+2-58-64 ° 7469 7430 7427 7451 M+1-58-28 Q 4(2+11,72 2254+074 Q U12237 о М+2-58-59 I о V335® 49 G 0 M+1 -58-22 50 p QY +10° +09° +08° o 7564 7455 1.1481 М+1-59-28 М+1-59-29 7604 о .7577 7583 Pegasus II Cluster 7501 7499 7503^ Q М+1-59-2 7452 U12255- U12451 • U12461 p ®DI М+1-59-27 е~М+1-59-41 ! U12494 7562 - 7SS7 7562А/?° ° 7591 М+1-59-15 OU12423 О • 7518 23h20m 23h16m DC» о 1.1474 Д ЗС458 М+1-59-9 ' p$DL 23h12m 23h08m 23h04m . U12266 о- U12224 0 PISCES 23h00m 22h56m U12213 О о U12196 PEGASUS +07° +06° 22h52m +05° 22h48m Stellar Magnitudes (V) фффффффф***** andbrShtw 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6 5 7.0 7.5 8 0 8.5 9 0 9.5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60’ Variable Stars • ® @ ® ® (•) ® ® (S) ® О Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag « Nova Q Quasar Д Radio Source X X-Ray Source Copyright О 198 7 2001 WiUmonn-MI. Inc
82 2 +18 +17 +16° +15° • +14° • +13° +12° I +11° • • c +10° 2h48m 22 0 e • A* 3C453 • • о e ,h44m 22 • • h40m 221 • • • ♦ • • B6m 22h • • • • 32m 22h ♦ 72830 ♦ .07 9 28m 22h2 • • • • 290 • • !4m 22h2 • • ♦ • 0m 22h1 e • • • • 6m 22h12 U11944-' • < ’ m 22h08 4 PEGASUS • • • m -18° • +17° +16° +15° +14° +13° +12° E> tir • • +10° • • • • • • • • • 7291 • +3-57-11 • • <s • • 7272 M+3-57-6 • • ^7280 °PX о • • • PS 7244 0 • • • ♦ • • J °U11928 • 9 M+3°56-17 • M+3-58-2. • • • • • о • • • • • • • • • • • • • ♦ • • • • © • • • • M+2-56-25 9 • - • • • • • • • • • • • • • . • • • ♦ • PZ • • • • • • • • • • • • • • • • • • ' C428-65 о C • • RS о U11952 428-63 о U1 Q_l_ ♦ U11921 . о Y о • 948 • • • • V • • ♦ cs • V • 2233+134 • • • • • • • • • • TX о • • 7236. ♦ о 7237 M+2-56-21 о • •о M+2-56-2. • • • 2 * • • 46^ • ° QS • • • • • • • • • • • • • • • ‘.PY • 31 IN ♦ • «О • RU • • • • To • • • • //2/84 * . .o . Л4+2-58-9 ° ^7372 —7?7Л 0 7348 • • 7347 ♦ • 7346 • 7305° • • • • • • • • ° (/12017 • • • - • • • • • о • U1 • . s 1.5177 1947 / J/U ™ 7366 • • Л4+2-5 M+2-58-2^ • . - ф Hom 42^ • 8-1 am • • • о 7328 • • • • • • • • • • • • • • • • • • • • • • • +09° - • +08° h M+2-5 • • 3-3 C429-22 . • • • • • • • • . » • © C404-13 •>PU • • • • • c • • M+1-56- 0 U11987 г 21 • I • M+1-56-17 О • • • • +09° • - +08° • • , 7362 * U/2/j • 0 ‘^U/2/33 8 U12074c • • • • • • • • • • • • 9 о AT • • • +07° - +06° - • • • • • • • • • • ♦ • . U12054 ♦ • • • • • • • • • • • • ♦ • • • ♦ • M+1-56-16 * О - +07° - +06° - +05° • U12178 4) • • • • ♦ • • • • • 9 • • • • • • U12021 (2404-4 9 • •• • •DH • • • ♦ • • • ф 26 в • • Biham • +05° L • • 9 M+1 -58-6 PEGASUS • • • ♦ • • О 7312 • ^7311 • • — — c U12023a PWo • ’ • ° 30 • • © PQ • • • • • • • • • 22h48 m 22h44m* 22h40m 22h36m 22h32m 22h28m 22h24m 22h20m 22h16m 22h12m 22h08m □pen Star Clusters and Asterisms Z) О o to scale < 5' Globular Star Clusters Ф® e to scale < S' Planetary Nebulae -ф- -ф -ф- о >30” 30’-10" 10" 5" <5" Bright & Dark Nebulae ° ° to scale 10*-5’ <5' Galaxies 0 ООО >5 5’-2‘ 2-1 <Г to scale major axis c“ 22h08m to 23h28m PEG to scale +18° tO +05° PSC WH Tmon / tony ft^jopnrr / WJJ Remakhn
83 2 +1f +17 2h16m 2 . U1194 • 0 2h12m 22 4 • • • • h08m 22 OY • M+3-56-9 • h04m 22 . о 7177 • 100m 21h ♦ , • • ♦ • • 56m . 21h —* • • — • • 52m . 21^ • • • • <13 • I8m 21h4 9 • • • 4m 21h4 • s2141+175 • jm 21h3( PEGASUS • • • 1-18° +17° • +16° 72* +16' ♦ 14 . ;aU1192< • M+3°56-17 . ^7206 7207 Uli 908 о • • • • • • • .от • ♦ • • • • • • • • +15° • • • 5 M+2-56-25 • — • • • • • • • si • U11896 ♦ • • ♦ • • О 1.1427 • • • • • • M+2-55-24 \M+2-< , ъ M+ M+2-55-25 ‘ • ’ ° 1.5145 U11821 15-23 * * 2-55-22 • • *GH • • • ♦ ЛЗС437 • • • • • * +15° +14° + 14° • RSc U11952 C428-63 0 f 1/1 Q- < U11921 ° Y о • 948 •. © • • • • • • • DF ^2147+145 A • 3C437.1 U1?820 • 0 и HN® • 11803 1.139 00° о • • • 4 ‘ C427-7 + 13° 7236 , ♦ 7237 M+2-56-21 о M+2-56- • • • 22 ' • ♦ • > • • • • • • • <20 ‘ M+2-56-4 0 . e 7159 • • • • • • ЛЗС437.1 • • • 4+2-55^8 ' • • • +13° +12° +12° •o • RU • • • • • • • To . • • • • • • • • 7195 . e 7194 • • • 0 • • 17 • • • AG о 7138 • oTU • C. 7113 • °7112 • • • 7094 -ф- • • • • <□ • +11° о • U1 о/-5777 © 1947 C428-29 21 * • • O 7190 U11865 * • • • • • • • • •* * • • • • • • • • • • • +11° +10° +10° • • ♦ • • • .7212 . ♦ i 7193 о U11871 /V • • • • 1+2-56-3 ♦ • • M+2-55-26 1 0 • ♦ • • 7Ш C42"9 • © • • • • • • M+2-55-5 о V • • +09° • • • M+1-56-17 Cj • • • M+7-56- 0 ♦ •—o— . M+2-56-6 • 1 • • • • CM+1-56-6 . ♦ • • Enif< • •° 1.1398 • Me • • • EE< • • • > • - +09° • +08° • 0 AT • • ’ • • M+1-56-14 • • • • • • >19 • • 1.1414 • • • • • • ♦ • • • 7 • • <?7inl U11782 00 7101 • • • - +08° +07° • ♦ • • _• • • • M+1-56-16 * о • • • M+1-56-4 •( 0 )S ♦ • • - • • 0 M+1-55-10 .♦ * • • • ♦ ♦ • M+1-55- • - +07° +06° •- •DH • • • • • • • 26 0 ф Biham M+1 -56-13 о • • 0 V 18 C403-5 о • • • • • U11846 • t 4C+0 • • • о M+1-55-13 • • 6.69 • • • ♦ • • • • ♦ • <3 • °7102 • • н +06° • +05° - • • • • PEGASUS • • • • • ’ .22V • - • • • * ♦ • • > U11851 ° M+1 -56-1 • • • • • • • 1 •^7 U11792 • • • ♦ 4 ’• • • • +os° 22h16m 22h12 !m 22h08m ♦ 22h04m 22h00m 21h56m 21h52m 21h48m 21h44m • 21h40m 21h36m Stellar Magnitudes (V) • ••<•••••••• 0.0 2 5 30 3 5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 atxi brighter и.э Double or Multiple Stars < • ♦ Individual members are plotted il separation exceeds 60" Variable Stars o® Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. о Nova Q Quasar A Radio Source X X-Ray Source Copyright & 1987-2001 Wiltmann-Bell, Inc
Open Star Clusters and Asterisms ' •' ( ) 0 x b.,1’ to scale < S' Globular Star Clusters ф Ф Ф to scale < S' Planetary Nebulae -0- <> 4 < >30" 30’10" 10" 5" <5" Bright & Dark Nebulae □ lLj □ ::: to scale 10 -5' <5* Gc A >5 to scale ilaxies О О о 5-2' 2-Г <Г major axis Galaxy Cluster •f xi to scale 20h56m to 22h16m +18° to +05° PEG EQU, DEL Wil Tirion ; Barry Hapfxrport / W/ll KanuWus
21h00m 20h56m 20h40m 20h36m 2Oh32m 20h28m 20h24m DELPHINUS о MY . + 17 C448-33 + 16° C425-36 О © + 14° +09° 7003 + 10° 20h48m J ® 20h44m |.'7 M+2-53-7 o \ M+2-5 3-11 RS 9 a C447-3 +14° 16 U11587 M+2-53-9 + 11 ° 6988 6972 U 578 C399-26 о 69 17 +08° >14 6969 U 6 0 +07° MZ U 1155 <=> MS +06° 13 +06° AQL . C3 99-28 MR 20h52m 20h48m 20h44m 20h40m 20h36m 20h32m 20h28m +05° m 6906 +12° 6944 'Z 6944A +09° + 10° +08° +07° +11° 21h04m +18° - Uli 66° f ~ M+3-53-9 , ° I О NR «NP +12° NO U11638 U11634 6950 +15° P59.7-18.7 C425-7 10< DM EQUULEUS DELPHINUS •nv Uii623q p6956 Da o| ♦ U11620 M+2-5 3-10 U11659 C400-17tf • : • C4( : ° 10-12 • • • • • • • • < • • • • • UH639° • • • • .SV • • • • о 6971 • • • • • • • • O^S a • • * ! л m NN ъ I U11611 U11552 M+2-52-25 U11599 U11605 U11602 7K . C424-33 -6928 - 6930 ^6927 6927A cz°- * M+1-52-13 L/N593 6934 oMQ MP 1 (J1 1568-UH564 о М+2-52-/ 1111572^ Ъ U11571 M+2-52-6 DELPHINUS U11555 +05° 20h24m и b Stellar Magnitudes (V) • ttttti***** 0.S 1.0 1.5 2.0 2.5 3 0 3.5 4 0 4.5 5 0 5.5 6.0 6 5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars -> ♦ ♦ ♦ Individual members are plotted it separation exceeds 60" Variable Stars • © ® ® @ ® ® (•) ® ° Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag 4.0 mag. » Nova Q Quasar A Radio Source X X-Ray Source Copyright © 198 7 2001 Willmann-Belt, Inc
84 19h44m +18° 20h20m 19h48m 19h52m 20h16m 19h56m 20h12m 20h08m 20h00m 20h04m SAGITTA • 6839 P56.8-6.9 20h24m + 18° DELPHINUS +06° ® 1 з vz Ro V335 © V343 1.4997 • 6879 ♦ + 6° C447-3 о VI357 C423-2 V1473 6858 ° V346 00 8339 '• +08° +08° VI 339® C398-3 V 475® +07° © V1474 U11523 AQUILA 19h48m 19h52m 19h56m 20h20m 20h00m 20h16m 20h04m 20h12m 20h08m Alshain 60 p r ----+06° +09° +07° Ul 1522 U11524 I -♦ +05° 19h44m V1463 49 +05° 1 - 20h24m soy Tarazed 0 • Iе • • • • » --- e KQ. • 6891 k-RW—• • • ♦ • KL V1472 • <•> ♦ A ♦ VI422 ” • о # • • • 2016+112A,8 +10° +09° SAGITTA RU U11512 VI470 V733 AQUILA +16° 6840 6837 52 Я + 12° 47V C424-2 ° лЗС4Н Ul1543 • C398-2 * V1466 <•> 54 0 +10° DELPHINUS U11532 V1481© • Ul U11498& U1 1493q о U11482 • “VI465 • • • • • • • • • • SY ♦ • 48 W Open Star Clusters and Asterisms 1 > Г') Q to scale < 5' Globular Star Clusters ф® Ф to scale < 5’ Planetary Nebulae -0- -ф- < -Ф- >30" ЗО’-IO" 10"-5" <5" Bright & Dark Nebulae <2?o □ D - to scale 10’ 5' <5' Galaxies 0 | ° ° ° > 5 5-2 2-Г <1* to scale major axis Galaxy Cluster o to scale 19h44m to 21 "04" +18° to+05° DEL AQL, SGE, EQU M Tmon / валу Rappoport / WiH Remaklui
85 19h52m + 18° ,— 19h48m 19h16m 19h36m 19h32m 19h28m 19h24m 19h20m 5 ОС SAGITTA PS1.0+3.0 Ro 1 3C400.2 . P51.0+2.8 + 16° 4-15° VI466 <•>- + 10° +09° ' \>491) 6P P53.8-3.0 -Q-‘ ® V343 V338 +16° P51.0-4.5 RT- Be 43 ' Ta razed ° VI459 V 447 °RV 00, 6804 +09' { 8339 +08° +08' +07° VI458 +06° +06 AQUILA 19h48m 191144m 19h16m 19h40m 19h20m 19h36m 19h24m 19h32m 19h28m VI293 +15° 6807 ©V450 19h44m V341 19*240т P54.4-2.5 + P53.2-1.5 Be 47 &P51.3+1.8 + 14° V339 V340 AQUILA P52.2-4.0 • 4811/ 52 Я 8340 54 0 8339 <-P52.9-2.7 P52.5-2.9 P51.9-3.8 . King 26 8337. V889 Be 45 . P50.4-1.6 P48.7-1.5 2400 46 8336 8334 P4 8.0-2.3 LDN 684 28 (VI208) VI339® о U11482 »VI465 47 X • i ’• MS V925 V1456° 31 b Do 35 29 0)2 25 0) 8143 • 8333 LDN 673 8142 . P45.9-1.9 3C399.2 . <>6803 V1463 B338 8335. 38 Ц P44.3-5.6 • *°V1261 &P46.3-3.I P45.4-2.7 V1457 V342<> 8332 8331 P43.0-3.0 V1450 : B330 A 6781 8140 19h12m +18° P49.4+2.4 P48.7+2.3 P48.7+1.9 + P48.1+1.1 VI448 • P40.4-3.I +14° .+10° —I +07’ +05° 19h52m — +05' 19h12m 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 85 9.0 9.5 9.7 Stellar Magnitudes (V) Double or Multiple Stars Individual mernben are plotted il separation exceeds 60" Variable Stars • ® ® © © ® ® © ® (•) © 0 Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag 4.0 mag « Nova Quasar A Radio Source X X-Ray Source Copyright© 1987-2001 Willmonn Bell, inc
Open Star Clusters and Asterisms to scale < 5' Globular Star Clusters фф ® to scale < 5' Planetary Nebulae Ф < < >30" 30" 10’ 10"-5" <5’ Bright & Dark Nebulae <z?<2? ° D ° to scale 10 -5' <5‘ Ge A) >5' to scale laxies О о о 5-2 2 -Г < Г major axis Galaxy Cluster ; '» to scale 18h32m to 19h52m +18° to +05° AQL HER, OPH, SGE, SER Wi< Iff юг) / Burry Rrjppupurt / Will R&naktoi
86 1 + 18 8h40r2 ] 0 • • 8h36m 18h32m 18h28m 18h24m 181- ’2( )m • 18hl6m 18h12m 18h08m 18h04m 18h00m * i 1 QO +17 V999 * ’ » о . 1///30/ • o M+3-47-10 • • • • •e • °V992 • • • • • • • • 1 • • • © IQ • ♦ • • • • • • • • • ♦ • • >6555 ’ U11107 о • HERCULES • ♦ • •0V91 Г 1 и '5 +17° 93 • х1 A0 +16° • • • • • • • • • • • • • • ♦ • • • U11242 о • • • • • • • • • • • • • • • • • • • • • • ♦ • • © V980 • • ♦ • . • • • • +15° ♦ • ♦ • • -• z • • • °V997 • • • • • • • • • • • • •V991 * 1,6627 • • • • ♦ • • • • • • • M+3-46-21 ♦ e 9 9 9 l 6574 • о • © V981 • . • • +15° +14° • • • ♦ • * P44.3+10.4 • • • P43.3+11.6 V996 • 6635 . • • • • • о ♦ • • • • c • 1PHIUCHUS- ♦ • . ... • • • 9 • • • • 6570 * • ♦ • • • V977 • • • • • 9 О +14° • +13° • • • ♦ 4 • • • • • ♦ • • • • • • ♦ • • : • • M+2- • ° 6615 . • 46-12 • • c,U11168 • • ♦ с • • • • • A 4C+13.66 • +13° +12° +11° • +10° +12° HERCULES • • • • • • • • • • 1 • ♦ •® RX • • ♦ • • • ♦ ‘o’ U11214 • • • • • ♦ 9 9 • • ♦ • 0 • • • oU11141 • • ♦ • • • ♦ • <3 +11° • a • • • . 1 ► • • ♦ • • • • • • • • • • • • • ♦ • • • 4 • a— • « • • • • • • • • • • • • • 1.4688 0 • • -t—— • • • • 3C368 • A • • V2118 © • +10° • • . * о U • • 1293 ’ .. • •>-- . V451 • • • • • • • • • 1821+107 • • ♦ • • • • • <>P38.2+ • 12.0 • • *• • • • 9 • • • ♦ • • • • • • • • • • • +09° • • • • • • • • • • • • ♦ • • • ♦ • ♦ • ♦ • • • • • • • • • • ♦ • • • ♦ U11122* 9 • • V839° . . • #72 • • • • • • • • +09° • • +08° -©-X • • • • • 2 _ • • Ф V2393 • • • • • • • • • • • •• ®V2291 • • • • • • • • • • • • • • • • • • ♦ • 71 • •• • • 1 •J • • • +08° • • +07° - • • • • • • ♦ • ♦ • ♦ • • • • • • • ♦ • • • • • • • • • • • • • • • • • • • . M d •. c ♦ • + 1-46-4 C-56-8 . (J11093 +07° OP +06° (- • • HIUCHUS • • • • • • • • ♦ • ♦ • • • ,♦ « • • SERPEN • • • S CAUDA • • • * ( • • I • 9 • 11177 •< • • >6572 • 9- • • • • • о 0 • V2300 * • • I - +06° 1.47. к • • • SerX-1 * +05° >6 ’ • . • • *. QV *. • °. • • w • • • : t__l_ • •©QU • ER • •и • ♦ < • • • • • • • • • NW • •• • • • • • • • • • • • • • • • e • • • • • • • • • • • • 9 9 • OPHIUCHUS • • • +05° 18h40' 71 18h36 m 18h32m 18h28m 18h24m 18h20 1Ц1 m 18h16m 18h12m 18h08m 18h04m 18 hoom 0.0 and brighter 0.5 • •< 1.0 1.5 2 Stellar Magnitudes (V) !••••••••••* .0 2.5 30 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 • • • • 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted it separation exceeds 60" • ® ® Amplitude 1.0 mag. or less Variable Stars @ ® ® (•) © ® ® ® ® Amplitude Amplitude Amplitude 2.0 mag 3.0 mag. 4.0 mag и Nova Q Quasar A Radio Source X X-Ray Source Copyright О 19Я7-2001 Willtnann-MI, Inc.
86 17h2Om 17h24m 17h32m le^OO”1 + 18° !--- 17h28m 17h36m 17h40m 17h56m 17h44m 17h52m 17h48m V656 . UZ ««V964 I. J 268 V961 GO 0 6389 4C+16.49 U10950 CII3-1 +15° M+2-45-7 U10985 4 M+2-45-5 V624-®-. U11001 +14 +12° о V914 °U11073 V2386 s э M+3-46-6 ®z +10° U10941 • о •o U10919 M+3-45-25 64V M+'3^26 o. 6375 ^ui0872 6347 V657 ® V642 U10864 C83-11 4C+13.65 1.1255 V2388 P3 6.0+17.6 ° RU +09° ® V2114 V2377 ’ +08° V564 +07° V2300 1.4665 ° 6509 ° C56-I +06° C55-20 OPHIUCHUS V2379 U11074 0 A 3C363.1 +06° +07° +09° C56-2 ° C55-4 -C55'2 Л ?6378 °U10868 HERCULES . U.X 93 +16° OPHUCHUS ' U11055 U11057° U11067 • RT V2387 ° Л => U10981 U10913 56 • <54 Rasalhague ©V2380 U10918 1/10862 е' RV- M+1 -45-2 V640 6368 - V2370 U10844 C54-27 U10805 Io HER U10802 +10° i+08’ +05’ 1 - 18h00m V566. I —0—1—•- 17h56m 17h52m 17h48m 17h44m 17h40m 17h36m 17h32m 17h28m 17h24m — +05° 17h20m Open Star Clusters and Asterisms О О О to scale < 5’ Globular Star Clusters ф ® Ф to scale < S' Planetary Nebulae -ф- <> < <> >30' 30M0' 10" 5" <5" Bright & Dark Nebulae D a ° to scale Iff-S' <5‘ Ge >5 to scale laxies О о о S'-2' 2'-Г < Г major axis Galaxy Cluster ; 'i to scale 17h20m to 18h40m +18° to+05° OPH HER, SER Wil Trion / Barry Rappoport / iViH Remoklus
87 1 +18 +17 +16' + 15° + 14° • +13° +12° <□ til" +10° 7h28m 17h24m !7^20m 17h16m 17h12m 17h08m 17h04m 17h00m 16h56m 16h52m 16h48m _ . • 1.1 Q • • • • 0 • V65( • • • • • • • • ©V942 • • • • • • • • • • • в • • • • 1.4 • • 0 М+3-13-5 • 624 . V918 ® • +17 +16’ +15' • +14' • +13 +12' +1Г +10с +09' Ф • V640 -• • © • • «е_ • 6347 • • М • • • • о оАК <-3-44-3 . • V873 • • • • • ♦ • • • •тт • • • • • . (2110-12 . . 0 о • V920 . • • о * • 'Л • • • • • • • -♦ • • DoDz7 • • • • • • • • ♦ ♦ • • • • • .• 49 (V8 • • • • • • 23) HERCULES OPHIUCHUS • • • ш • • • 9805 Rasal • • • gethi 64 а • • • • V451 • • © • • ^0 • • • • $ . i • «• ♦ • • ♦ • • • ♦ • • С82-15* • о • • • • ♦ < V933 * . • л • • • • • • • • • • • 0 М+2-43-2 • • • • • • • 0 1.1255 L. ♦ • • * • ♦ • • • • • • • . °U1( 60 • • ♦ • • 685 • • • • • • • • ,, 6368 • • • и 10802* • • V438 ‘ . л • 0 М+2-44-1 • • 0 U10705 • ♦ • о V2359 • • • . • ® V235 >6 • • • • U10844 о • V2370 • <• • е • • • V2369 • • ♦ • 37Ф • • • • • • — о- • • 1/70699 . • • • • • • • ♦ • • 251 • 1 • • • • • +09° - ( +08° 1- • • ♦ • • • • • ♦ • • • • • . U10720 о • V2365° 0 ф <281-18 • • 0 U10674 • • • > • 27 К © • U10569 Ч • г • B V2114 ’ • • • • U10797 ° С54- • U10743 • • • • • • • • ♦ • • • • • • ♦ • • 1.4621 * • • • - +08' - +07' Ul 086 +07° - +06° - • +05° * • э 2 • °С54-27 • • • • • • UJ0789 0 • • ♦ • ♦ • ♦ • WZ • О 0 М+1-43-9 ’ • • • • • • • • • • • • • • • • • • • 47 k • • • • • • • • U10775. °и U10779 ^vdBUI * • 10778 • • • • ♦* • • ^U106. 6280о /23°6\ * • • 59 • • • • • • • . ’ 622 622 • 4 э 9 5 - +06' 5 I • * +05' 6h48m • • • • • • • • ± м • • • • • • • 6 U10738 • • • • ’ • • • 1656+053 • . OPHIUCH US HERCULE • • 45 ±3C348 Hercules А ] 17h28m 17h24m 17h20m 17hl6m ’ 17h12m 17h08rn 17h04m 17h00m 16h56m 16h52m Stellar Magnitudes (V) • ••••••••••• Х* OS ’ 0 I S 2.0 2.5 3.0 3.5 +0 +S 5.0 5.5 60 6 5 7.0 7.5 8 0 8.5 9 0 9 5 9.7 Double or Multiple Stars • • • - Individual members are plotted if sepaiation exceeds 60 Variable Stars • ® ® ® ® ® (•) ® ® ® ® ° Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag 3.0 mag 4,0 mag. в Nova Q Quasar Д Radio Source X X-Ray Source Copyright О 1987-2001 Willmann-Bell. Inc
87 16h48m +18° 16h44m 16h12m 16h40m 16h16m 16h36m 16h32m 16h20m 16h28m 16h24m о V915 i да U10490 A2159< • q ° 6073 1.1209 +15° Pal 14 • M+2-4M4 о QI 3C334 6084 0,1310249 o- о C109-35 о U10405 • 6078 o 6074 M+2-41-18 +14° U10287 о 6083 0 I M+3-41-141 • -|7K -------------<+i7° M+3-42-8 M+3-42-26 U10412 6113 24(0 C79-89 UV 1.4593 29 h 1.1206 C79-85 45 0 C80-19 M+2-41-10 +08° V897 C53-2 +07° 21 о C52-44 C52-29 41 • M+1-42-2 ?X 451 C52-38 C52-4 HERCULES 16h12m 16h16m 16h20m 16h44m 16h24m 16h40m 16h28m 16h36m 16h32m Ci U10463 C52-21 $ +09° +07° +08° U10414 о ° U10416 M+1-42-5 * +10° +06° c>6224 °6225 +06° I + 11 1.1196 i C79-62 о- I 6106 О U10337* •’ HERCULES 3C346 • U10388 +16° +15° +14° + 12° + 11 +10° +09° 6219 +05° 16h48m V600 ® AS U10380 U10360 C80-17 о V892 . A 3C347 U10387 C53-4 V907 1635+119 M+2-42-7 C52-51 33Y® C80-46 ° M+2-42-3 6142 О 154 13 28 n V746 о C80-32 6081 о 1.1205 • 12 C52-19 16h08m • • • i : SERPENS : CAPUT U10239 U10238 i. : о» • — 1.1199 4 U10225 о . 47 FS о PY 1.1197^ +05° 16h08m Open Star Clusters and Asterisms to scale < 5' Globular Star Clusters ф ® ® to scale < S' Planetary Nebulae -ф- -ф- -ф- < >30" 30" 10" 10’ 5’ <5" Bright & Dark Nebulae □ ° - to scale 10 -5' <5‘ G< >5’ to scale ilaxies О о © 5-2 2’-Г <Г major axis Galaxy Cluster ; i to scale 16h08m to 17h28m +18° to +05° HER OPH, SER Wil Tifton / Barry Rappoport / WiN Remaklui
88 I6h16m + 18° 0 0 +15° + 14° + 13° +12° 15< 0 + 10° +07° +06° +05° ।-- 16h16m 16h12m о 6084 С108-138 6057 16^08т ^^6055.' 16^00гл ~/6056^ 6044\ о > 6030 8 * М+З-41-141 • •> г-'.:/ 2 A2159 ". о V892 q 6073 Pal 14 О 7k 15h56m 15h52m 35 К®15h48m 15h44m 15h40m 15h36m SERPENS CAPUT 5996 &5994 'A2108 1.1178 6042 /Hercules Galaxy Cluster A2151 • L • 6034 с М+3-41-47 A2152 M+3-41-95 o- U10204 Cl 08-117 • О 1.1151 U10093 . 1.1135 26 T8* М+3-40-18 . I о 5977о 5972 _X1— 15 M+3-40-12 U10287 о 6083^ 60™ о 6074 М+2-41-18 О U10249 • 0\ М+2-41-14 U10239 U10238 11198 : о о о' 0 1.1206 C79-85 С108-59 M+MMJ м+3-41-29 l| о U10I44 ^М+3-41-28 О М+3-41-61. - -U10134; 2'.___\_^'U101_43 М+3-41-124 Q........ U10201 I о С108-81 \A2147 1.1165 . :о*. -1.1155 . 1.1174 —a___ U10169 ъ U10164 ^М+3-41-64 C79-48 C79-40 0 6066 О • °6065 1.1169 о О U10176 М+2-41-2 6029 0 С79-37 О I M+2-41-3 о C79-47 p U10158 M+3-41-3 0 I • ^ 6022 4 о 6018 41 у #6012 *№0111 }U10061 U10077 19 V О 5980 oR U10068 ^ ,, М+2-40-15 6009o 6006 о 1.1149 f С7919 6007 • О C79-8 1.1141 ’ 0 C78-80 U10037 5962^, U9925° 18Г» • +16 29 31 V 0 U10014 U9996 0 о 1.1133 I о ' U9951 17 V ® +15 4C+14.60 Q о 1/9991 С? 5984 M+3-40-9 M+2-40-9 +14 @ 20 X U9941 о 5970 ° 1.1131 +12 ;I.H96 Т • о NQ oU10213 ’ 13 M+2-41-6 46 > 6081 о PU C79-18 M+2-41-10 1.1205 +09° c® 40 FP 5997 +08° 1.1197 27 k 0 U10023 - C51-5 24 a • 6017 • 0 6014 0 U10042 5988 C78-64 0 U10225 о . 47 FS С50-113 112____ :/. 1199 • 12 oPY M+l-41-6 PX U10029 ° U10147 U10041 •° U 45 43 .°U10146 HERCULES 16hl2m +10 —tr- 6063 16h08m 16h04m M+2-40-10 16 +09 U10130 U10137 5983 +08 16h00m 15h56m 15h52m 15h48m 15h44m Stellar Magnitudes (V) зпЛчМе 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60" U9964 Unukalhai M+1 -40-10 U9978 5960 о 09976 о С50-59 5964 С50-68 SERPENS CAPUT 15h40m Variable Stars • © © ® © (§) ® © Amplitude Amplitude Amplitude Amplitude 1.0 mag or less 2.0 mag. 3.0 mag. 4.0 mag. +07 +06 - +05 15h36m »> Nova Quasar A Radio Source X X-Ray Source Copytighl C> 1^87-2001 Willmann Bctl. Inc.
15h36m 15h32m 15h28m 15h24m 15h20m 15h16m 15hl2m 15h08m 15h04m 15h00m 14h56ni T 1 о +17' 18 V • +16° 17T ® +14° +13° • +12° +11° • • 16 +09° - • 15 V • •_ • • • • • ♦ • • • • • • • —Г 42 1 SERPENS САГ • гт- 036 ’UT • • BOOTES • М+3-38-83 о M+3-38-81 o • 1.1085 ’ о . М+3-38-71 ; т • • • 1 о • И 7° +16° +15’ +14° +13’ • +12° |> • 1Т • +10° • O U9912 • • • ® ox в 12 T2 • • •=> U9846 • • ♦ о OU • • ♦ • M+3-39-/9 • • • >3-39-1 о M+3-38-84 О ~ 0 о С105-91 • • • • U9640 С7 • • • 5954 °5953 • • L_q • о M+3-40-1 • • 9 • 9Г • ♦ Cl 06-33 0 • • • • • ♦ • • • • • ♦ • • • • * 5951 M+3-40-9 о o’ 1)9900 * • • • ♦ • • • • • M+3-39-23 © oS • • • • ♦ • • • • • • о 1.1093 • • • • • • • • • • (77-125 0 • 1.1118 • • M+2-39-18 • • 9 о 1)9808 М+2-39-10 * . C77-5 9 о • • и • • )758 о • • C77-25 ° • • • -• ♦ • I • • м+< 2-38-31 • • ° U9919 oU9901 5957 О 5936 • • • • • M+2- о 5926 M*2 • 7 9 3913 ^°C77 61 -39-13A C77'63 0 C77 НПЗ 55 • • о • 5 M+2- • U! • • 852 M+2-38- 38-42 & ^38 >721 U9712 588/ • 39 -38 • • 5956 • U9897 4 • • • • <31—| C77-7 • • ♦ 8 • U9814 ъ • • • © FF • ♦ • ’ . М+2-38-33 U9654 • • 5782 М+2-38-29 ~ ° • 138 • • • • • • • °W 1522+ W - - ♦ • • • • 01 U9807 ♦ • • © 1)9794 (J97 • • 55 о • ♦ • M+2-39-1 °* ♦ • • U9675 ’ о • (76-133 » о • • • • • • • • • 1)9845 о • • M+2-39-28 о , .° C77-74 • ♦ о OP — 0 M-h о C77-26 • 2-39-6 /. • (77-11 1092 о ° U9708 • • • • U9614 0 ‘/.1079^ U9616^> । М+2-38-30 ’ _• М+2-38-24 078 - +09° 111 - +08° +08° - • • +07° - • • • +06° 596) +ns° - • (50-22 о • • * (77-130 о ♦ • /-'>42063 ъМ+2-39-20 odt/982? 1.1116 ♦ . M+2-39-8 . 0 • • 0 LV • • • • U9696 0 ’ U9685 о z • ч V • • • • о С76- о 5790 М+1-38-24 • (50-1Г 5944 • • * 5931 ° 5940 &5941 5942 • • 1)9844 U9838 0 ‘ 5920 • • U9798 0 M+1-39-l3^AJ9 9-14 A204(h'’'\ t (49-46 *.^ 799 о C4 JC313- M+1-39-3 о z ’ " \ ! \ Г »•••• . ^-'A20. 9-33 1 U9689 o к 4 • 28 • 9 УА2020 • • 1.1082 0 • - +07’ - +06’ - +05’ • • • / • • • • • • • 4 —z4 ',‘A2055 г 2052 ‘ ° M+1-39-10 .C49-21 ^42033 • С48.ц • • )0 • • • • о U9625 • • • . (50-25 0 5955 0 • e 1)9864 0 • ♦ • • о (49-148 • C49-150 о 5921 (49-115 • M+/-39-J6 A20 (49-75 °°U9781 SERPENS CAPl • 29,' ’С4 ъ I JT o/J/0/ 9-39 J9757 VIRGO- ♦ о M- о С49-3 о (49-1 ь -38-28 О U9667 • • 15h36m 15h32m ’ 15h28m 15h24m * 15h20m I5h16m^^ 15hl2m 15h08m 15h04m 15h00m 14h56m Open Star Clusters and Asterisms to scale to scale Globular Star Clusters Planetary Nebulae Bright & Dark Nebulae Galaxies <т> -ф- -Ф- <• □ <^0 О о о >30’ 30М0’ 1О’-5н <5" to scale 1 O' - S' < S' >y to scale S'-Z 2'-Г <1‘ major axis Galaxy Cluster to scale 14h56m to 16h16m +18° to +05° SER BOO, HER, VIR i IVrf Tman / Barry Rappoport / Writ Remaklui
89 14h24m +18' 15h04m +18° i—w 15h00m 14h56m о 1.1075 14h52m _r___0___________ 14h48m 14h40m 14h36m 14h32m 14h28m 1.1076 EQ A1983 « U9640 M+3-38-57 M+3-38-43 +16° + 15 о 1.4516 1)9558 . o . + 17° ° M+3-38-44 1.1085 M+3-38-71 “ C'?5’9' C76-84 C76-91 C76-80 oEN + 12° M+2-38-33 M+2-38-29 Q> U9654 =>5782 о M+2-38-21 + 14° + 11° + 10° +09° +08° +07° +06° M+3-38-35 14h44m 1.1050 1.1053 ° ’° C105-34 * °M+3-38-30 35 0 1.4483 о 29 К 0 1.4503 ®EK M+2-38-31 5628° 1.4438 BOOTES 1.4417 о U9444 • A1913 +16° о 1.4478 U9675 ' О • (76-133 о (76-92 U9614n • 0 c 1.1079 о, U9616 0^1-1078 M+2-38-30 * • M+2-38-24 . 0 C76-97 A2020 BOOTES • ° 1)9667 VIRGO +05° 1--- 15h04rn * o C76-1 ^ 5790 М+1-38-24 (48-55 о 5769 ° 1.1082 0 1)9625 (48-70 15h00m 14h56m C104-65 EL * о C76-77 * U9517 о (76-41 4 1)9561 M+2-38-20 5763 °o 5762 о 5736 • 0 C76-78 U9513 560C +14° U9273 U939< 0 C75-34 о 1)9374 1.1035 1.1044 C76-16 CK 1)9443 1)9249 1)9474 C75-108 5681 C48-19 U9492 (75-41 Л19267 • <p5644 5647 К 1)9389 ь C75-74 U9288 о\|.Ю14 o° M+2-37-8 M+2-37-9 _Q______ U9259 1)9500 о U'9530 1442+101 0 C76-34 0 <p C76-43 5758 I о 5759 5655 -------- 5648 g C75-56 +15° 5747 о + 12° M+2-38-8 09523-^, M+2-38-7 U9521 ° M+2-38-5 U9534 о i • о 9 32 C76-10 0 (75-110 C76-58 U9555 i о (48-22 . о (48-43 5765A ______° 57658 ___ 14h52m 14h48m U9411 ©NW U9364 о NS (47-116 о U9471 1)9454 I о C47-142 M+1-37-50 Q. 5701 14h44m 14h40m 1)9356 +11° 5666 C75-81 5669 M+2-37-11 5627 U9286 о +09 DW ° U9225 ’ . Of • ° ” ' 5665o о © • 1)9339 C47-60 • • • • • • • 5645 • О A 4C+07.36 ♦ • — 56798 5679C ! o56/4 ° о* 5679Д ♦ 09400 U9385 14h36m 5661 5652 NQo U9i38 C47-56 14h32m 14h28m +08° +07° (47-37 U9246 ’ 0 U9244 +06° +05° 14h24m Stellar Magnitudes (V) 0.5 1.0 1.5 2.0 2.5 5.0 3.5 4.0 4.5 5.0 5 5 6.0 6.5 70 7.5 80 8 5 90 95 9 7 Double or Multiple Stars • • ♦ • Individual members are plotted if separation exceeds 60" Variable Stars • ® ® (g) ® ® ® ® ® ® ® Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag 3.0 mag 4.0 mag. n Nova Q Quasar A Radio Source X X-Ray Source Copyiyhit) 1987 2001 Wittmann-Bell, Inc.
14 +18° +17° +16° +15° +14° +13° +12° +11°. +10° +09° +08° +07° c +06° - c • h24m 14 ' 0 * A1899 • • • • о 09206 °DV . . ° 5600 • 0 5587 • ° 5591 ° 5583 12om ]4h #\.999 1.1000 % U9167 • • • 20 • ® CY • • • • • ' C74-159 16m . 14h • Q 09126 . M+3 €103-120 о м+3 09121 * о о 0 09110 * <.5522 • .5525 qU9117 • • • о 5 М+2 йк 12m 14h( / о» ? 1.982 1 ° СЮ. 5490С о • о °5490 09078 М+3-36-54 ° ♦ М+3 -36'73 о 09043 36-72 ° о 5504 • е 09067 о м+з-36- . 1/9055 1.979 ° С10: ’ ’ 0 U9C • • • ° €74-129 505 -36-53 )8m 14h0 1-86 • © • DP \ М+2 36-47 о. €103-65 с & М+. ° М+3-36-52 с 63 о М+3-36-50 С10 -87 44 5454 ° 08996 " ’ • ’Z 5459 0 о 4m 14h0 - • © • 36-44 J8987 И6-38 О -- 4С+16.39 М+3-36 U89 у U8977 • • 0 3-55 ♦ • • 274-77 Muphr 13h5< • • i • _ • • M+3-36-25 • -170 * 92 <• 0 08872 U8883 ’ •j-967 . • C74-130 1.959' • d ф 5m 13h52 • 7 о U8839 1.960 ’ °M+3-3* ЛД 5332 • A 3€293.1 . M+3-3 -36-7 • 2 о 08827 M+3-35-34 /946 । 1.948 0°!, M+2-3. M+2-35-24 • m 13h48 . • T ♦ Cl 02-5 ’-35 ° M+3-3 s'33 a 51) M+3-35 • • О 1.944 S-22 • 1 • • • П 13h44r — 1 + BOOTES 8o • 4T 5-27 + 0 5293 — • —H 4 ♦ M+3^-35-22 26 • • • • • • 8< n 18° 17° -16° +15° • +14° ♦ +13° +12° E> tll" - +10° • - +09° - +08° • ) - +07° • — +06° 0 - +05° • • 555," ' • 14 • 09104 • М+2 • • М+2-36-39 и90 36-42 0 о . • U9025 с • С74- )2 • 74-76 78 o0 08907 "c74-28 • ♦ C74-30 1.962 • • о DO • 4C ♦ • A +12.50 • • • 09177 о 5562 о • • • • • • • " * ?00TES 557! • 5563 o • о 5573 5599 . • CQ о 5575 NN C47-75 o C47-74 ° ♦ 5665Д ъ • • 01.994 0 o°55 1/9162 5S- • • 09134 o— • ^09169 • Al 890 • °- C46-9/J <^5535 €46-81 ‘ . 5543 - / 5546 0 о 5542 a * 5538 • ° 5549 0 5537 5554 • * • &3C298 9 • °. • о 5551 • • • • 09089 ♦ 31 2 • ♦ 15 М+2-36-49 °. • М+2-36-54 •“ГТ— М+2-36-52 * С74 SS" ° К28 М^36-24 * е М+2-36-57_ • &5514 ° 5519 • • ♦ 09041 €74-124 о • • • • • • ° €74-126 • • и М+2-36-45 ° - -136 5482 09084 274-135 0 С74'131 . 5487 О » 0<- 5491 о ♦ • • 0 • ♦ • С74-103 0 545 О М+2-36-30 i М+2-36-33 0 ( 09008 0 М+2-36-41 0 о €74-94 9 о , • 5446 а 543 ° 5437. 5463 U896 9023 ° ° 1/9007 54 1/9015 п м+2’36 С74 1/8995 ° Л/ • • • 9037 • •— 5470 . Ок • €46-56 • • 6 * OU8973 • » U8972 • 5414 С74-43 >5436 « ^Г5424 о 5409 1 ^54315423 23 &U8948 64Г «5.’ 1 • U8 1+2-36’21 0Л 0 М+2-36-10 ♦ • • 5417 о • ° • 5418 5405 • 0 08966 • • 08 С46-33. M+2-36-2 ♦ ° 1 0 08878 • ♦ 918 0 €74-20 • 0 C46-17 о oo €46-25 08896 _ CP 5384 o’ 0 5386 5382 . 5374 5387 q e . €46-1 906° о /.966 ° 5373 . 0 • • • J8861 • • • • • C46-5 0 • 0 ‘ • C45- e • • • 0 C46-2 • • 2 5363 5356 O(J8818 p /о 533 ^-’3 5348 <./> • • о DM • 08769 • 0M+2 • • i • 125 . 08 M+1- ♦ • -• ♦ • 8 \1809 1 — • • .0 C73-72 • • ♦ C73-71 о • -J5-18 ♦ — • • • 728 08708 3137 VIRGC • 9 U8689 • ^HT +05 L 14h2 4m 14h20m 14h16m 14h12m 14h08m 14 ’04m 14h00m 5364 5360 1 3h52m 13h48m 13n44m 13n56m Wrl tinon / Barry Huppupurt / Will Remakkn
90 13h52m +18° r - 13h48m 13h44m 13h40m 13h36m 13h32m 13h28m 13h24m 13h20m 13h16m BOOTES о 5217 Cl 02-58 о 5158 KR® 4T M+3-35-27 5172 ’ 0 1.894 J 5332 о 5151 о М+3-34-40 ° 5293 о М+3-34-26 + 16° 51) 1882 4 1.881 1)8452 +15° 1)8383 5125 U8385 о • 5180 4C+11.45 Q 1)8425 о -v.---- 1)8370 M+3-34-28 о •Oo 1)8535 KT 1948 1946 У So^.al,944 + 14° * М+3-35-14 ШЗ+176 M+3-35&3 f М+2-35-16 С73-72 U858S + 10° +09° FP +08° BOOTES С45-74 08572 +07° 08626 08613° 08427 5118 +06° . 08532 4C+12.50 a 1)8450 0 U8689 - ' 1)8617 • 1)8728 1)8708 ............c.... M+1 -35-37 Л73-71 5179 -^"* ‘ 5178 °* 0 M+2-35-18 0 T 08596 M+3-35-22 Q 1331+170 ° M+3-35-6 1.858 o 1.857 +17° 5249 M+3-35-26 о DM DH 5248 08614 0 •-O'* 5239 СОМА BEREN CES o* 5222 5230 1.901 1)8563 С73-29 о • 1.900 V---- U8575 5209 oo °52 5235 ъ 5224 О C45-18 U8569 VIRGO +05° ------- 13h52m ®НТ 08657 U!_6.62^ ° ° 5261 0 C45-26 13h48m 13h44m 13h40m 13h36m 5162^ 0 5165 5191 O5174 71» С73-10 5208 0 13h32m 70 5115' * 5136 5167 5186 C101-31 5132 5137 5129 5185 ^J181 LQ о U8322 С72-41 5058 5100 59 е о 5080 VIRC0 5020 +16° +15° +14° +12° * о С72-23 1)8298 +10° • 64 13h28m 13h24m 0 1)8296 +09° 08382 °5071. °505 5075 • C44-67 • 4C+07 A • • U8285 32 C44-33 • FH U8349„ 5060 / C44~-36 5027 • • • @60 0 • • • 13h20m 13h16m +08° +07° +06° +05° 13h12m Ф LN о Stellar Magnitudes (V) • ••>••••••••• 0.5 1.0 1.5 2.0 2.5 5.0 3.5 4 0 <5 5 0 5.5 6.0 6.5 70 7.5 80 8 5 90 9 5 97 Double or Multiple Stars Individual members are plotted if separation exceeds 60” Variable Stars O®® ®)®® (g) ® ® (•) ® ° Amplitude Amplitude Amplitude Amplitude 1.0 mag or less 2.0 mag. 3 0 mag 4 0 mag. и Nova Q Quasar A Radio Source X X-Ray Source Copyright О 1987-2001 Willmann-Bdl, Inc.
13h12m +18° ।— 12h48m 12h52m 13h08m 12h56m 13h04m 13h00m 42 a 36 38 1241+176 27 3C275.14C > 1.827 +16 U8081 COMA BERENICES 1/8085 4935 29 0 1.3806 ^471° 4866^ *U8091 04758 A • 3C277.2 M+3-33-22 VIRGO о 4969 о 5020 +12° о +10° +09° +08° +07° +06° 12h44m 12h40m о I U8114 0 4880 о M+2-33-38 0 . U8032 41 <Ь 4746 U8253 о о о 4992 U8255 0 1252+119 С72-18 U8192 о КХ 0 4754 4762 о C'C72-13 C72-15 о <272-7 Q 1307+085 U8233 +05° - 13hl 2m 47£wVindemiatrix • J-840 C71-100 о o| . U8170 . 4C+09.45 . ЗС281 5 C44-7 \ ’ U8204 - 13h08m 4733 U8056 M+2-33-49 ' ° U8093 U80U 4779 12h36m 12ь32^ ^.3530 | + COMA BERENICES ' 25 • * 0 0 M+3-32-82 0 4595 1.3658 O o| 1.3637 4633 4634 =KN 4571 28 • U7979 . о 4498 0 4502 4 4515 +16° U7857 ° о 4611 0 4689 ♦ 0 4659 • • i.3W " °4639 4654 <? KM^e 1.3611 о 1.3718 1.3720 о 34 4694 4620* . °l.810 4640 О 4641 4584 0 7|/.3631 1.3635 1.3672 ^,4n67°l6 • о 46071 4647 04621 M 59 4649 M 60<3 o 1.3665 | 4637 ^38 ° 1-3653 4660 ° 1.3652 0 1.3727 Q 1.3773 01-816 U7942 °* М+2-33-44 С43-127 а 0 U815S СО ЕР 0 4698 CNoO M+1-33-33 ^4803 о 4795 U8045 00 U8042 32 FM d2 U7943 М+1-33-29 о 4713 oRT 3C43-48 о 1.3704 1.3686 о 30 P ° KT о Л4+2-33- 2 ° 1.3754 13h04m 13h00m 12h56m 12h52m 12h48m 12h44m 1.3647 U638 О 4540 о 1^0 ^4523 1.3522 1.797 z> . 1 CO . 4516 I о 4501 M88 4548 M 91 1.3478 a 1.3476 Q 0 4506 1.3501 1.358У....... 1.3486 о 1.3475 И.3457 e 1.3540 ф 4552 M 89 1.3586 4579М58 • 1.3608 O4608\4696 4598 0 4623 0 4612 <31 d' M+1-32-133 ^4551 о «4550 l3489 , 1.3459 +12° 4564ъ i Siamese Twins 4528 » o _qI^0 • '\3499 1.3481 1.3470 d4503 .110 4578 о M+2-32-161 1.3617____ О U7802 о 1.3518 Q* 1.3517 о 20 ’ 1.3468 .....H +10° 1.3487 Q4522 +09° л 4519A 4519 । 4535 M+1 -32-111 О 07688 й. C42-153 ’ 4Л 8 • 45188 4526 +08° °4570 о.>Л/С1 R ОЦ7795 | 18521 ® Q (.3591 ’ о 4588 4591 12h40m +07° <3 1.3576 °4580 M+1 -32-108 ° 0 4532 °U7739 0 4543 12h36m +06° VIRC0 —1 +05° 12h32m Open Star Clusters and Asterisms О О О to scale < S' Globular Star Clusters ф ф Ф to scale < 5' Planetary Nebulae >30’ 30-10" 10--5" <5" Bright & Dark Nebulae <C2<j ° l-j °1:1 to scale 10'-5* <5‘ Ge >5' to scale laxies О О о 5-Z 2-Г <Г major axis Galaxy Cluster to scale 12h32m to 13h52ra +18° to +05° VIR COM, BOO Wil Tinon / Barry Rappapoa / Will Remaklui
12h40m + 18° - 12h36m 12h32m 12h28m 12h24^ о 1-3530 IY®- + 17° + 16° ЙГЙ 4595 +15° 1.3637 + 14° KM -jo# 4611 0 COMA BERENICES ‘ 25» • 4450 0. 4571 11 1.3611 о 1.3583 44980 лллл о 4489 4502 4515Q о 1.796 О4540 0 1.800 1.3522 ^4S23 ^1.797 . 4516 О 4548 М 91 1.3478 о 1.3476* 0 • 1.3635 1.3631 0 12h20m 4344 о 07399А о М+3-32-30 4350 4340 о 1.792 0 о • 4383 . 4405й * * /.3365 - »1И^4^^4321 М100 I.783A °1.783 • 4396 & о О 4379 4421 4322 0 4312 12h16m 12h12m -^-07186 12h08m 0 1.3638 + 10° +09° 4598 о +08° +07° —O- 1.3392 Л4501 М88 44'4<"Л <5x^4468 4506 1.3501 о 4477 4479 44730 07346 О М+3-31-94 099-16 о • 07331 4166 ° M+3-31-61 & 07074 07073 07100 12h04m 4048 12h00m — ------j +18° окм+з-31-15 4040 07327 о о 4239 4237 4584 • 69M90 p4531 О_________ 4419 о й 4377 ’ 4446 4447 1.781 ° 07436 (Р4298 4302 о 4262 О 1.3096 о © M+3-31-49 • • M+3-31-6 M+3-31-75a 07230 * 0 • *3 3 U7194 4128 0 Q. 4152 M+3-31-41 С) 07109 • Q> M+3-31 -28 М+3-31-25 07032 0 ? 07196 6 04192M98 ° 4186 A1474 M+3-31-30 +15° о U7016 ) 4254 М 99 1.3077 < 07355 о 1.3065 о 1.3023 07003 о 1.3091 -----а ^1.3061 1.755 069-29 О 1.3019 -о----- +14° ^4212 i3044 1.3062 0 1.3059 о -1.771 COMA BERENICES 1.3094 1.3344 The Eyes Markarian's Chain 44584435' 13355 о ф4402 —гу 4406 М 86------------------ 4387~о ^4374 М84 1.3303 4388 q>4189 4461 . о 1.3540 " о 1.3475 <=>4552М89 13457 4486 М 87 44868 Virgo А 'у с^4476 1.3459 ° 4^86А 4478 • 1.3586 4^!^> 13489 4550 1.3393 0 44^8 4425^ %4Гз 4440 4436 РУ 4431 о . 1.3311 1.3109 4222 --•о 4216л ___0— 4579M58 • 1.3608 т 4596 4564 ъ 44^/^5iamese 4568 Twins 4528 13481 > о о1.3470 01.85Ю У05 • а1.3499 Jo 4486А 4478 . , "-------—1.794 . 1.3381 . 4497 • О 44$] 4452 *01.3413 1.3418 ъ 1.3331 vl.3358 ° 1.3356 b 4429 4578 М+2-32-161 1.3617 ---------- 07802 20 | -• о 1.8468 4482 о ъ 1.3425 о 1.3371 1.3518 о* 1.3487 4442 q 1.3517 о 4522 &4519A 4519 M+1-32-111 о 4535 О 07688 ----_____ 4445 4451 о 4483 °4570 ^_1U7795_1 .^ 1.3591 с> 4588 4591 4580 0 +05° L-• 12h40m VIRGO 4306 ‘ 4305 ‘ 1.3258 4351 o>4371 0 4313 4294 4299 0 о ^4330 ^4352 о 4390 1 НМ 4380 ^4417 ° 4424 <3 4360 Я 1.790 4410А, 8 C69-120 1.3078 „ О ъ 1.775 4267 1.3099 1.3105^ * 1.3100 ,4793 ;.42О6 -4168я4165 01.3033 J.3029 4164 73О21~. о 1.3008 07043 -0 4037 VIRGO 0 '.3127 о о KM 01215+113 /.3158 4325 °о 4320 М+2-32-25 М+2-32-22 4316 1.3167 О 1.3170 4307 о 1.3107 07307 —о--- • O/.3118 1.3151 AG ^1)7249 13046 1.3060 13036 1.3039 о ° * 1.769 Ъ о 4200 «Kt 01.3074 о 4207 * 1.3156 44 1.3211 <=>1.776 07383 4488 0 4472 М 49 4492 о Z 4356 07424 и7590 э 0 О 07596 '7 ^4411А 4 А" 44118 • А1541 0 4415 4434 £07580 4178 • 12 1.768 ° о 1.767 О 1209+107 4124 °SU 1.2990 о 4082 4083 * о • 4078 4067 0 M+2-31-10 + 11° +10° 4464 4465 4467i~*—^4416 M+1-32-76 * С42’153 q4518 U7686 0 • 4518В 4470 ° • 4466 ° С42-120 4526 07557+Я 4430 О 1.3576 г * ’CI '' 1.3521 М+1-32-108 0 4532 °U7739 0 4543 12h36m 12h32m andbrighw 0.5 1.0 1.5 2.0 2.5 ° 4318 1.3271 . 14353 *07567 1.3322 4366 I.3322A 4365 1.8267 1.3414 о 4453 4432$ 07085 M+2-3 ©X -27 M+2-31-20 <0 90 oM+2-31-18 KK о 07239 о 041-50 q4191 t)4180 pM+1-31-20 M+l-31-19 1 8 Л • 11 М+1-31-10 4029 " +09° +08° 1-3148 о o 1.3131 4276 . 4233 4224 О . 4334 . О 1.3259 ^.4341 ^4309 ^0 4342 _______ - 1.3218 4297 ^4296 О~ 4343- 1.3268 1.3225 . 0 07423 4333 ^39о1р4826 4269 0 Mil-32-56 4423 ° о 4376 FK M+1-32-41 12h28m 4^8 12h24m Stellar Magnitudes (V) 4247 4246° Ъ __________4235 M+1 -32-6 z, O4241 1.3115° i- о 042-9 •) 4215 +07° ;4260 0 1.773 • • 1.3155. 1.782* 4287-* .4282 4^оо * • 4281 , 12h20m 0Mi1-31-53 4264 <Т)4261 L 0 4257 .4266 ^ о 4249 [У4270' 4252 Ж°О4259 7р268 о *4197 М+1-31-30 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 +06° M+1-31-9 M+1-31-13 12h16m 12h12m 12h08m 12h04m — +05° 12h00m Double or Multiple Stars Individual members are plotted il separation exceeds 60" Variable Stars • ® @ ® ® (•) ® ® (•) ® © Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag 3.0 mag. 4.0 mag и Nova Q Quasar A Radio Source X X-Ray Source (.opynght © J 98/-200/ Wilhnann-MI, 1гк.
i; +18 !h00m 11 h56m 11h52m 11h48m 11 h44m 11 h40m 11h36m 11h32m 11h28m 11 h24m 11h20f Т1 18° 17° -16° 1-15° +17‘ 1 +16° I +1 s° • LEO i • : U6913, • • о U6891 L • • U6741 ‘ о • 3806 -о ? 380238 М+3-30-38 ° О М+3-30-44А !• лС97-35 0-3790 5768 )1 U6631 0U6614 • • • U6483 о с • 3659 с 3686 • ’ LEO • 71 • • с + 1 « • o\4014 о : WXo M+3-31-7 • ; c • S M+3-30-125 Cj • • ♦ 95 о ♦ U6911 *3934 V933 1/6794 О • • °С97-167 • • о t 3853 с • • • <>-*—•— • U6686 6 о 3828 • • U6655 U6666 ^176653 • ,+3’30-33 3°767 • о 1)6594 . U65 * U6586 0 ♦ 90 • о U6556 59^ М+3-30-11 ° 0 • М+3-30-7 3691° • ♦ е85 • 0 368/ 81-е- • • AF 0 3655 • — — 4 • . FP ?ЯЛЛ с //ЛЯ?/ ° M+J-JU-/// —. М+3-30-15 • • U0J00 л^2?лел 3799 jt +14° +13° c +12° г +11° +10° • +09° Л c +08° - । 4.07° .3996 • • oFZ °C97-179 ♦ ♦ • • 94 [i Denebola е- *. • • О U6753 ’• • • U6669 • • М+2-30-17 0 • • • • • • >88 • FS • ♦ • + 14° • 0 3623 М 65 6 +12° +11° +10° - +09° - +08° > - +07° ь M+x COM VIR 2-31-7 • • • • C68-81 * • U6775c U6758 §3872 О • • • • • • ♦ АК о • • • • •0 • . . /.2934 • 1.2873 о . • • /. 1.2826 ° 1.2804 0 — ’ •— • .2787 3628 - 'f 2782о . /2776 ° Тф°( _£763 о J • • • 3973 . ЗС267^ _ ’ о 1.736 • ♦ :^'^A13S 3908 • >0 М+220-31 • 0 М • ♦ о 1.2945 * +2-30-9 3773 . 0 • * ^ 3731 • ♦ • • • • • • а 3627 Мб • *• • ^3968 • ♦ • • • • • • • 3810 • 0 АН • • • « • • <! • . 1.2846 • ) • .2822 о е о 366 » • — 6 ’• • • a • • • U6871 о • • М+2-30-42 . о 068-76 • 3869.. 1-727 ° 0 1+2-30-35 ; " о м+2-1 U6740 3848 • э 3839 ♦ 0-21 3819 3820 о* "^3817 °« fj822'“J« 3833 ?ях 47 • о • 1.2941 • • • ф 78 1 4012 • • • • • • • • • • 3876 U£71 U6734 <? ’ • • • 7 /.722 А 171 б U6617 9 • • • • • 3692 . о 3705 о 1.2857 •1.698° № 1.692 | FR /.2853 . , . 1.2850 | * • 4029 • • бе • • 44 1.72 • 3863 о . ► \| о о ° 4 01720 • М+1-30-12 31.718 * 1 (0® • • • ^Нб9( ли 1.2871 9 U6 1.2828 1.2757 462 • • 4о IY 1.748 . • • • • U6804 • 040-42 © > 3843 • )А1362 ъ М+1-30-7 • ♦ • • о о • • 12830 +v / ~ 8 Л +06° > 9 • +OS° - • • <s • 3976 C40-54 М+1-30-18 о U6886 — о 0 040-51 • О М+1-30 3914* . • • • 16 ©3V • • • • • • М+1- • » • 30-2 Л • м 4+1-29-48 о + 1-29-42 JC39-/67 77 0 - +06° • 15 +05° М+Г-ЗГ7 c • М+1-31-2 С4 L • 0-53 • о • • • • • • VIRGO LE< • э | ° С39-162 Д ЗС257 М+1-29-. 12h00m 11b56ln • llhS2m 11h48m 11 h44m *11h40m *11h36m 11h32m 4h28m 11t'24m 11h20 UP Open Star Clusters and Asterisms d О О to scale < 5’ Globular Star Clusters ® Ф Ф to scale < 5' Planetary Nebulae •ф- <> -Ф- ♦ >30* 30--10" 10"-5" <5" Bright & Dark Nebulae <2?O? □ lj □ ::: to scale 10'-5* <5* Gc >5' to scale ilaxies О О О 5-2' 2-r <r major axis Galaxy Cluster ; 'j to scale 11 h20m to 12h40m +18° to+05° VIR LEO, COM Wil I mon; Barry Rappoport I Will Remaklub
92 1 +18 +17 3691 + 16° 85 • +15° +14° +13° +12° 1 h28m 1 0 1h24m 11h20m ,..,^11h16m 11h12m l1h08m 11h04m 11h00m 10h56m 10h52m 10h48m — 11 Q° LEO 36. • 3686 0 0 f.; 3684 59 Q> . • • 71 « • М+3-29-24 о 3t 1.2703 ° U 0 M+3-29-25 505 5296 3602 ъ Q о 3592 3598 • • • 0’ М+3-2 0 06157 С95-104 0 3501 8-56 • * о 3487 c ° ’ M+3 M+3-28-52 -0 • • • '28'45. 8478 U6 8474 № C95-70 3457 }443 ° 0 ff3454 035 K3455 О • 05945 • ♦ Г 1 и 3370 0 +17° • +16° • +15° +14° • • +13° 13 ? M105 + 12° + 11° 18-10 • +10° +09° - +08° °| ° 3681 81-e- • 0 3655 • • • ♦ • * о 06300 • ♦ • • • 4 • С+16.30 06137 а • .<95-91 о ; о) 06112 ^^A114 06104 • M+3-28-38 ° • • 0 • ’ \ ^3447 Al 126 3447A • • 0 M+3-28-26 • 3405 3399 ♦ • • •AF • . FP • • • 0 C96-28 70 0 ф Chertan • • • • • 0 • • • • • • • 06043 о Iе M4 • • 3-28-22 M+3-28-11 • 05950 FS • • • ♦ • . °3596 FK< ♦ • М+2-29-2 С95-106 0 • 0 М+2-28-5 Г 3485 M+3- • • 28-36 • • . 3391 3419A /2 • • /. 1.2826 • ° 1.2804 0 •— 1.2787 • 1” 3628^ 2782 о юте T;; 12763^ 1 /• ’0 • ’/et Л 12684 . V ° 0 2666 »73п • М+2-29-4 " • . М+2- о • 5 '9-3 C66-1°7 34- • • • • oW • • О 3419 • O3412 oU5944 C66-28 „ • • > " 3627 M • 3623 M 65 66 о 1.2708 • <• ► о 3593 • • О '677 • •С67-7 06206 о 1.2628 М+2-29-1 • • • 06169 0 • M+2-21 0 • 8491 о 6 • 3-46 06078 M+2-28-24 • C • /. (_/ 9 \ C66-4 3384 ъ 66-36 о 3389 о 3379 548 о. <a 1.2846 ‘ +11° + 10° 3692 о 1.2857 \/ 1.698 о<№'. 2822 о • о 3666 • • 1.2681 ° 1.2674 о • 1.2649 О е 3559 • 06231 © FI • 0 3524 • О /V 35f6 0 C66 ♦ • • +2-28-40 -94 • • • • • • ► 781 • • с • • 1.2638 о 1.2634 % • 1.2672 о 06248 0 ° М+21 3547 • ♦ о 9-5 .. • 06093 о 1.664'^ 3492.^ У a 06081 о • • 1142 o 06072 343 о 3444 ‘ о C66-62 n М+2 ’ «531 »EY ,3433 • 1.692 • .2853 . 1.2850 •FR • • • ♦ • • 1.2637 1.676 0 С67-91 С67-18 • • • • ’ -AM ♦ • ♦ M+2-28-29 0 о о ’ 3467 = 3490 3476 • ° 3477 0 . M+2°-28-26 U59 3466 U6014 94 • • 3428 0^3429 • /б" 1.696 1.2871 0646. +08с к • +07° - • .2828 •’ ? . . /.2757 • • • 061 о О М+2-2 8-4 9 • • • • 30 0 C66-104 • 06062 C66-71 ° C66 1.658 ^ %M+2-l C38-64 о . 0 M+2-28-27 zo 3439 ° -68 >8-31 М+1-28-16 о } С66-47 О3425 . ^3417 ^>3427 °М+1-28-14 • 12830 • • • • s 06312 1115+080А, 3624 *<39-113 С39-104 • 0 вс М+1-29-15 • 0 • • 0 С39-22 '06185 о С38-118 06168 63Х 3526 о е СЗ CUO f. ®\.,'IA1149’ 8-107 L. C38-78 0 C38-68 • ♦ Ant Goloxy , 3t62 U5999 0 • 3441 • 0 ♦ • J v - - +07° • • +06° t +05° М+1-2 +06° - +05° — • 9-42 o ( Ф-’67 77 0 • • С39-80 о 0 1.678 С. 0 06233 * С39-16 19-59 . С39-14 'п С88-10 1-670 C88-I0 ъ • 01.669 М+ 5^ C38-103 J-^8;"59c> • U6046 о -28-25 ° U6066 M+1-28-22 • о • 956VY • US923° LEO : sextans' • • 3 - C39-162 • A C257 о М+/ -29-35 • • 3601 1 М+1-29-1 * М+1-29-17 ° М+/-29-Ио,^"1 2^3567. °С S’ ,--'6062/0 -"\С39-43 С39 39-9 06141 АР- °° 15 . • • C38-96 о • G • ^53 Q3E 06049 * p C38-5L 0 ’ • 06068 -48 ° • iO 3423 • • 338 11 h28 m nh24 m 11h20m 11h16m 11h12m 11h08m . 11h04m 11h00m 10h56m 10h52m IC 1Ц1 )h48m • • 0.0 and brighter 0.5 • • 1 1.0 1.5 2 Stellar Magnitudes (V) .0 2.5 3.0 3.5 4 0 4.5 5 0 5.5 6 0 6 5 7.0 7 5 8.0 8 5 90 9.5 9 7 Double or Multiple Stars Individual members are plotted if separation exceeds 60’ Variable Stars • @ © © © © (®) ® ® @ ® о Amplitude Amplitude Amplitude Amplitude 1 0 mag or less 2.0 mag 10 mag 4 0 mag и Nova Q Quasar A Radio Source X X-Ray Source CopynqhtC) 1987-2001 Willmann-Bell. 1гк.
1 +18 J +17 +16° 1 +15° j +14° 1 +13° 3384 3389^ +12° 0h48m 10h44m 10h40m 10h36m 10h32m 10h28m 10h24m 10h20m 10h16m 10h12m 10h08 r~ J 0) о ОС E LEO 0 3370 0 • • М+3-27-63 * © U5651 о • • С94-390^и56 a323\ ° M+3-27-14 9 • 39 • ♦ U5552 • • • 3154 • 0 C93 ID- -57 ? ° ° 4 36 +17° ф-зоп +16’ +15° 6-30 +14° +13° l+12° • 0 ’ 1.639 • M+3-28-5 °°EX • • ♦ • • • • 50 . • • • М+3-27-65 • M+3 • • c • 27-45 * о Q94-56 о 1.607 9. М+3-27-2 о М+3-27-3 о ’ U554 7 • • M+3-26-48 • • ♦ • C93-5! 9 °M+3-26 • U5495 • U5858 • M+3-27-75 ° Q 1.635 • • • 1.616° • • • M+3-27-53 М+3-27-41 • • •ER • • c> U5526 • • • • •33 • • • •—о 52 k • 335 „о 3377A о о 3346 7 EV о • U.V 3300 • 0 • • • 9 46 ES • DW° U5633 0 U5646 0 . 42 • C65-18 • • • M+3-26-44 1/5477 M+3-2 • ^3377 *3367 • • • ♦ .° 33^8 о( о . UZ ‘ U5832 • 6S'82 U5760 ° C65-62 . • 0U5739 • /V • • M+2-27-14 +2-27-13 Q C65 • U5644 • \ • • о • -24 U5627 • 37 • • C64-106 OC64- • • • 01 • *34 • • b 3379 M 105 • • • U580 C^3C245 . •C65 J 0. 3306 8 • 69 0 * 3299 U5735 . ♦ • • М+2-2 о US695 3253й °M+2-27-23 7-24 ‘ ♦ / I • 1 ') A999 / Фо /Ш595 • • • • • 3153 0 3134^ •EQ • U5470 . Leo/О . М+2-26-29 л I +11° r • 53 I • +10° 0 3368 M 96 о U5869 о U5897 P 3351 M 95 о C65-78 * • 0 <= U5737 3279 • • . • U5642 • • • • •— • - oM+2-26-33 • *• V W • 32 a : o Regulus E> *11" >+10° - +09° - +08° М+2-28-10 • • ♦ • • о C65-73 0 М+2-27-33 • • / 1 \ • • .-I O 1 \1.б1з: . ' — 'A1016 • . । --'A1020- Leo Cluster a3217 • A V ♦ * • • 1.595 1.596 31 9 d 1 9 +09° • +08° - М+2-28-4 о • • • 3332 o • • • 47р<* 45 M+2-27-S 0 U5616 9 • • • • • о 3130 1 C64-85 © • • • • • 0 • • 49 ТХ • C37-55 ,} О • l_ Ji «® 44 0 • • C37-38 o0 7-39 • • • M+1-27-2 0 Z • г -.37-5 • • • • • J +07° - • 1 +06° - \ V +05°o - * Л'"' • °U5892 • • • • ♦ • С37-78 • 48 6 — C37-67 ’ * • • • • • • C37-24 * • • • • • • 9 • • 1602 0 • о U5537 U5522 0 C36-51 0 C36-49 3C237 - +07° • • - +06° • 3356 оо .о 3362 • • 0 3376 М+'' 3349 ♦ M+1-27-26 U5818^ 27-29 ° &4C+06 41 • С37-82 . а • С37-81 • • • U5687 ° C3i • iC2^ C37-28 • • • 43 • M+1-27-3 3186 M • • • ./36-8^ °U5573 9 + 1-26-28 • о C36-67 • 3C238 LEO zk * 9 >16 ♦ • ,ях SEXTANS 5о0 1.634 • • _214' 1337 • ° М U"88 1628 3326 о _ + 1-27-20 • ° С37-87 • • + • U5702 о • • • • о C37-11 ♦ • • • • • ^36-72 9 ♦ C36-52 ’0 oM+b M+1-26-11 26-16 +05° 10h48 m 1oh44m 10h40m 10h36m 10h32m 10h28m 10h24m 10h20m 10h16m 10h12m 10h08m <• □pen Star Clusters and Asterisms О О о to scale < 5' Globular Star Clusters ф ф Ф to scale < S' Planetary Nebulae >30- 30М0' 10--5" <5" Bright & Dark Nebulae <2?< / □ ° to scale 10'-5' <5' Galaxies Galaxy Cluster Q О О о / >5’ 5-2' 2-Г <Г to scale major axis to scale 10h08m to 11 h28m +18° to +05° LEO SEX wt Гтоп I fonyRoppop&l/ WiN Rfmokkn
93 10h16m + 18° --- +17° + 16° О + 14° 37 0 +12° + 11° - + 10° +09° +08° LEO 10h12m 10h08m DD 3154 •о M+3-26-48 C93-57 C93-59 ° • о °M+3-26-36 U5495 U5526 •33 M+3-26-44 0 U5537 + 07° |s----; M+1-26-28 +06° 30 T] U5453 U5477 c M+3-26-30 O3!2! °3119 10h04m XY- 1OhOOm a U5385 3094 о C93-19 09h56m 09h52m ° I.S82 C92-58 3041 3060 U5343 о ° I 3053^ oi048 C92-62 U5274 09h48m 09h44m 09h40m 09h36r о U5213 2949 293-3 * I 2923 M+3-25 o| 2943 2941 ' XT 2928 C92-45 ° °I581 C93-18 b C93-15 о U5342 U5344 1.572 8 1.571 о 1.568 о U5234 P 1.565 C93-13 e26 о M+3-26-6 о M+3-26-7 C92-59 U5258 М+3-25-27 C92-35 ° 3075 °C92-72 л 3C228 • >34 • C64-58 RY 3107„ о U5400 'I C64-26 3153 0 3134 * EQ M+2-26-33 U5522 - C36-67 «06-72 ' +05° । - 10hl 6m -C64-607 1004+1300 о U5470 U5454 . M+2-26-29 n , 32 a Regulus —o— 1.595 1.596 о 3130 C64-85 M+2-26-23 °EP о U5456 31 C36-51 о C36-49 3C238 ..A.... C36-52 ,o • 16 3C237 C36-27. • 14 10h12m o M+1-26-16 M+1-26-17 10h08m M+2-26-12 0 M+2-26-8 3080 Q> U5395 . Ъ M+2-26-11 tb-— ------- 1.585 C64-28 ’ 27 V aAt ?M+2-26-13 M+2-2S-53 0 U5324 M+3-25-38^ P221.5+46.3 , * • ’ M+2-25-32 c C63-83 * 23 C92-37 ° J________ о M+3-25-23 16 Ш- U5232 0 C63-62 °' 2954 3C22SA • °C63-32 C63-34 ° • М+2-26-17 о C64-27 о M+2-26-16 ° . U5358 о О C64-18 aa<^ M+. t 3020 291 ^3019 •3024 ° 3016 • 0 2-25-49 • • • ♦ 21 M+2-25-52 M+2-25-23 ° о 1-555 C63-21° • 19 • 18 о U5409 U5396 o • 1.584 *. 3$69 ff1-577 C64-20 * ° ° 3070 1-578 • M+2-26-3 q ♦ ---------------о____________ C64-9 C64-19 29 Я M+1-26-4 1001+054 01 U5432 Sextans 8 U5373 ' 10h04m 10h00m 09h56m 0 M+2-26-4 1.569 ’ IRAS 09371+1212 -----Frosty Leo Nebula q . 29580 U5177o M+2-25-19 °' U5173 US 164 % M+2-25-14 M+2-25-28 I о 2984 o + M+2-25-10 ° M+2-25-54 °DV о C63-79 M+2-25-51 | ’ M+2-25-34 0 1.557 ‘ • ♦ • ♦ 0 • . 1.552 • ♦ • • • 1.559 140 ^3049 U5270 М+2-25-42 C63-61 U5267V i 0 —I—о-------y—tQ- U5?86 M+2-25-391 M+2-25-37 M+2-2S-36 M+2-25-35 • U5308o/b U5304 C35-75 йС35-82 • RR 0U5288 3C227 ’ C35-57 о ® I C35-55 09h52m 09h48m 3C226 < Io U5204 z M+2-25-21 <> • U5189 О C63-27 •• ° 2940 °2939 §U5215 C35-44 US218 2990 +( о EK M+1-25-15 SEXTANS 09h44m 2948 о 1.551 C35-23 . HYDRA : 2962 : 0 09h40m +( 10 LEO OU +( 09h36" Stellar Magnitudes (V) • •••••••••••« 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8 5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60" Variable Stars • ® © ® (•) © © (•) ® © Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. « Nova Q Quasar A Radio Source X X-Ray Source Copyright t) 19Я7- 2001 Wil/mann-Bsll, Inc.
9 09h36m +18 +05° 09h36m 09h04m 09h 09h08m 09h16m 2m 09h20m 09h32m 09h24m 09h28m • 8 +15° +14° 0 +12° +10° +09° +08° +06° OU +07° • 10 +11° 09h00m®FZ 08h56m • LEO • • • • • M+3-24-J M+3- ‘5 • -46 * • • М+3-24-24 о 83.-7- 2797 о U4925 2795 A- 0 M+3-24-29 • 80’ 1.2454 2794 0 2791 • • • ♦ • 78 • • 71> *D476\ • c • 0 U4729 • ANCER • • 2711е • — М+3-23-21 •» 17° +16° +15° +14° .U4670 ' +13° Л+2-23-11 +12° в - +11° *2923 M+3-25-3 ♦ • • • • • C9/-; °l Мн • 7 ’ ° GO °, oM+3-24 3’24-4< о W9 О 2819 \M+3-24-l U4864 • ♦ -36 07 3 . • ( • 3C215 273 S> 3K ' cliptic U472] 2730 • • • • • • • • н • • • • • • • у • __ «. - ” • oU4 962 1)4873 => M+3-24-17 81 V 1.528 • ♦ • C90-67 • 0 • ♦ • 63 • 62 0Ф • • M+3-25-1 • • ♦ • ♦ • • — • ♦ ... • • • 82 Я *Г oGM • • • l_ • 1.2431 o ♦ • • • ®ЗС212 • о Mi-2-25-9 • • » • • C62-22 Q> • 0 1)4931 . о M+2-24-5 • U4827 о -• CW • M+ M+2-23-27oo M+2-23-26 • • 2-23-24 . о * M+2-23-25 о Mi-2-23-23 ’ о • С61-31 U467 ;—о — • • C63-6 о • • • M+2-24-15 • 9P • • • « U5025 • °U5044 • • • • • • • 1)4861 О • • • • • • • .ОС61-32 U4694 °- • M+2-25-8 о • • • • • C62-29 2873 . о ' 2874^2872 0 U5003 • ♦ • о 1.530 • • • • ♦ • •• • • ^С61-44 . 2728 272. • . о * ф- Acubens 65 а 2720 1 о • U5082^ 2919 ’ • о 2912 2914(3^2911 ♦ • • • • • ъ C62-30 • < • • • 0 M+2-24 ♦ • • • -7 • ♦ • • >U4884 • • • • • 76 К • . * 1.526 • ^U47. • .. ° M+2-. RT® . ♦ \1 1 ?з-19 - +10° +09° - +08° —jq U5093 . • w 0 2913 • • ► 6 2 CO > • • • • ♦ • — • • • • • ,°l • J4845 . • • • • • c ©El • • 2906 3< • • • • U4957. • • • • \ M+1 -24-8 • • • • • • • • ^ 2731 • • • • • • • • • • 2894 3 C35-3 • • 2882 . • • • ®DF • • U4959 ъ • • U4S • о • ° • • C34-20 • • • • 2777 о ь 2773 JL- • • • • • • • • • J +07° • ф16 • ts M+1-25-3 • ° U5069’ ♦ ♦ • LEO • • ♦ CA NCER GL a 1)4890 • • 2775 • • • ° 1)4781 ’ • • • • C33-43 0 • • <^2718 о U5100 • • ♦ ^U5107 ‘ • • • • • • 2864 ° • M+1 -24-19 • г • 0 о M+1-24-11 1)4946 • f : • • • • • о U4797 • • •-18(0 • • • • • M+1- • • • • • 23-16 HYDR _J.O — • • А — +05° лоКг zm 09h08m 09h12m 09h16m 09h20m 09h24m 09h28m 09h32m m Open Star Clusters and Asterisms О О о to scale < 5' Globular Star Clusters ® Ф Ф to scale < S' Planetary Nebulae >30" 30’10- 10--5" <5’ Bright & Dark Nebulae <2?<;'j □ □ □ to scale 10'-5' <5* Gz Co >S‘ to scale laxies О о о 5 -2' 2 Г < Г major axis Galaxy Cluster •ч 'i to scale 08h56m to 10h16m +18° to +05° LEO CNC, HYA, SEX IVrf Ttnon / Barry Rappoport / W/H Remaklut
94 09h00m 08h56m 08h52m 08h48m 08h40m 08h36m 08h28m 08h24rr M+3-22-20 CANCER C90-33 • C8S ® X 68 о U4444 M+3-23-21 +16° + 15° + 14° о U4545 ° M+2-23-25 & U4599 U4670 • ° M+2-23-23 0 Л4+2-23-5 <^U4582 + 12° §C61-44 . 2728 2725 О О I о • »1.526 + 10° +09° +08° +07° HYDRA +06° ’ 0 U4590 2720 о о U4729 U4433 С* . 0 2593 ' 2596 ,.27// 132’0,,-- 1.2406 :> P208.5+33.2 0 1.2398 и468^-'Л • C61-31 U4677 —•---S-------r- 0 |_ 2734 o 4 Uml 25 cP 52 C60-13 © 27 BP C60-26 60 34 ф о U4452 +0 = 2731 •+0 +С U4594 С32-23 о С32-32 2644 ° M+1-22- М+1-22-15 • 36 c ‘ 37 2648 M+2-22-6 °C61- 7 09h04m + 18° -- Asellus Australis • 47 5 08h32m -@-31 0 130’ 3C201 3C202 U4639 M+2-23-24 . о •, U4731 М+2-23-19 CANCER . +05° ।-- 09hQ4m 63 62 0 • 54 1/4385 0 3C212 &3C208.1 • Q 3C208 3C207 U4550 • S 0 FQ 29 • C60-10 .^C61-32 U4694 M+2 -2 3 -11 ф Acubens 65 а RTo 1.523 Р219.1+31.2 М+1-23-4 ^ 2661 FX 45 TWo 2682 M 67 FW © 50 h 2651 C6/-2 о U4568 о 49 Bl b ® о 2657 FU- J C60-30 М+2-22-3 I о 2718 C33-43 M+1-23- ___ |o 09h00m 08h56m 08h52m 130 08h48m 08h44m Stellar Magnitudes (V) and^ter 0.5 1.0 1.5 20 2.5 10 15 40 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 U4552 о U4540 М+2-22-2 VZ М+2-2 C32-46 08h40m ’ 08h36m 08h32m C32-24 о 08h28m +С 08h24rr Double or Multiple Stars Individual memben are plotted if beparalion exceeds 60' • ® ® Amplitude 1.0 maq. or less Variable Stars © ® © © ® ® © ® О Amplitude Amplitude Amplitude 2.0 mag. 10 maq. 4.0 mag. □ Nova Q Quasar A Radio Source X X-Ray Source Copynght © 198 7-200J WiHmonn-M. Inc
08h24m 08h20m 08h16m 08h12m а.1Я° 08h08m 08h04m 08h00m 07h56 m 07h52 m 07h48 ♦ • m 07h44r n 18° 94 • • +17' +16° +15° • +14° • M+3-22-8 . 7 C89-16 • • • • • 1 • • • • • •16C • ► • • .2522 • • • • CANC • 3 • ER M+3-21-2 9 • • • • • • • • • • • • • • • • 9 • — + 17° • • U435C о • • • • • • • • • • • • • • • • ♦ wz * • • • 0 1)4190 ♦ • • 5 • • ♦ M+3-21-1 • • • U4139 • • • • U4090 • • 2454 • 9 • • • • 4 •16° 4 • • • . z • • • • ♦ • • . 2 .9 514 e • Ul • 9 2507 м+3 .O Q • ‘ 1)4170 • 0 O <=>1)4175 -21-7 . ei U4145 ’ 9 • ♦ • • • • • • • • • • • +15° I i о • Л 1)4385 .. ‘ • • • • • • • • • • • • • °C • • ’° M+3-21-18 1)4240 . . ♦ • • • ‘ 3C190O • C88-9 . о U4115 °‘ • C59-1 ‘ U4077 C58-69 0 • • * • 9 -Q • • • • • • ’ V3 — 47 +14° 1 • Q • • C60-3 • • • • • • • • • 12 ♦ • • • • ♦ о M+2-21-2 • ♦ • • • • • 1 • • • 1)4060 . • • • • GEMINI +13° +12° • +11’ ♦ , 1 Л0 • • C59-57 ’ • • • 8 • U4154C I I • • +13° • • • • • • • • • • • • • • • • • • . 1.2226 ° о 1)4216 ♦ • • > • • • • • ♦ 9 • • • CANIS MINC • )R ,• • • • » • • • • +12° ° C60-5 • • • R® • • • ♦ • • • <• • 9 9 • • • • ol • . C59-45 49 4244 • • • • M+2-21-6 • ♦ • • • • • U410 0 9i ♦ • 9* • • • • • • • 1)4006 , 0 +11° • ► 21 * • • • • • • • • • . * P2 • • •• • 1.9+22.6 ’ • • C59-42* "U4 U4215 о * 3C191S* C59-34' C59-17 211 ’ о . • U4198 [\oU4197 • • \l 9 9 • • C* : . • C58- C58-4 13 * • 5 ° • • • ne 458- • • • 33 • +10° +1 и • * М+2-22-1 ♦ • • • . • • C59-36c 0 9 • 1)4171 * о • • ф • Q 0754+100 • ♦ • ♦ • +09° • • +08° • • । Л7<> • • • • • • • 170 ♦ 0 U4276 • • • • • • • ‘ M+2 • . • C • • 21-10--'. 59-27 2513 ♦ • J^M+2-21 A10 2511 -5 • • _ф_Р21 1.4+10. + • • • • • • • —> - M+2-20-8 +09° • • • • • • • ° C59-5G • • • • • • C59-32 C59-37 ° C59-33 2526 • 0 0 • • * о 2508 9 • C31 • • • • • 16 . 2496 У ^2491 • • • • • • • • • • • • • • • • • • • • +08° 4 4 • . C32-14 °- • • • • • • • • • • ♦ M+I-2M6 . M+1-21-17 0 9 о 9 C31 -37 • • • о C31- • • ? . 2485 0 0 2499 • ®BU • • • • • • • 9 • M+1-20-5 Q • • • s U4025 • • °U4( • • • )05 +07° +UZ • ♦ • • CA • NICER U4183 o c M+1-21-5 • • • • • • 430-16 о M^l-20-7 » • • • HYDRA • CANIS MIN ; °C3i-65 OR • • • BW • C31-24 • • • • о BS • < • • о I • Л+1-20-8 C302 • о • o • 9 • • • - +06° • +UO • • ±Л(° L 3C198 • • • • • A о MQ • • • • • • • • • • • 1 .* .1t98 -u • 1.2231 : о . • . • • 4™ °U4228 • <= 1)4203 • 2504 • ♦ • = ® BV • • • • • • _• A • • • • Ю-24 • ux • U401 и • ° J +05° j +Uj 08h2 w * 4m 08h20m 08h16m •*08h12m 08h08m 08h04m др • ( )8h00m 07h56m 07h52m 07h48m 07h44m Open Star Clusters and Asterisms to scale < 5' Globular Star Clusters ф ф Ф to scale < 5' Planetary Nebulae -ф- >30’ 30--10’ 10--5" <5" Bright & Dark Nebulae □ □ °- to scale 10'-S’ <5‘ Gc A >5’ to scale ilaxies О О о 5-2‘ 2-Г <Г major axis Galaxy Cluster G to scale 07h44m to 09h04m +18° to +05° CNC CMI, HYA, GEM Wrf Tmon / Batry Rappupuit / Will Remuklui
95 07h52m + 18° —. 07h48m 07h44m 07h40m 07h36m 07h32m 07h28m 07h24m 07h20m 07h16m 07h12m • GEMINI 74 f C87-4 +10° +09° +08° U3805 : ° U3820 51 BQ <S> 67 Q 1/3772 ® N7 U3936 + 12° Do 26 U4006 U3755 U3839 M+2-20-8 zz- +0; • C29-25 +07° +0 C30-11 C30-20 U3768 +06° +0 UX 2350 ВР 0 U39OO ° V346 ’ U3974 C30-9 1 ’• ‘ °d. , C30-8 "2454 ♦ ° I о • 2418 0735+178 ©BN С87-21 U3766 +14 0 • • • • • • • • • • a • • • • 4J4O6O • • • • •• • CANIS MINOR • • * • • • • • • • • • • , • *(-58-43 C58-45 +05° 07h52m 10 68 oRY •© ОТ V347 1/394/ Q U3962 M+2-20-3 la 2416° i о . U3924 C58-33 U3 938 2433>A592 i о® C58-16 U3955 V344 3C181 Q U3877 ъ vx ® M+1-20-5^^4005 Q U4025 о C30-16 М+1-20-7 M+1 -20-2 ° BQ 07h48m 07h44* Stellar Magnitudes (V) 0.0 «nd brighter 0.5 15 U3892 C57-19°i Medusa Nebula . C57-16 GEMINI 3C175® ?2402 Gomeisa M+1-/9-5 QU3785 ' М+1-19-3 •.oBO U3738 +0' M+1-19-2 Procyon 10a •C30-7 07h40m * 07h36m 07h32m 2.0 2.5 3.0 3.5 4 0 4.5 5 0 5.5 6.0 6.5 7.0 7.5 8.0 8 5 9.0 9.5 9.7 . о C29-29 • • » • ••° • a • • a le 78 •• OU3819 a • • ♦ CANIS MH • • MOR *. ’ 07h28m 07h24m 07h20m 07h16m +0. 07h12m Double or Multiple Stars Individual members are plotted if separation exceeds 60’ Variable Stars S ® @ © ® (•) ® ® ® ® ® Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. * Nova Q Quasar A Radio Source X X-Ray Source J 98 7 2001 WiHmann-BeH. Inc
9 07h12m +18° 07h08m 07h04m 07h00m 06h56m 06h52m 06h48m 06h44m 06h40m 06h36™ 06h32m --- +18° 2304 ®NP U3635* 0 +17° . * о CR 4-16° + 16° © W +15° +14° +13° +13° +12° +09° +08° о U3738 +07° +06° . U3658 +14° <33 • 41 45 +15° 30 U3688 hi+2-18-4 ° U3641 RS 15S 16 2251 8 7 1.448 | -♦ +06° Bi12 V613 oV744 CANIS MINOR • V731 06h40m 06h44m 06h48m 06h56m 07h04m 07h00m 07h08m +08° +09° +07° <14 13 U3691<t> +12° +10° C29-3 M+1-19-1 +05° L 07h12m •o <5 U3707 о QZ © . QY 8e 29. U3602 • 1/3578 оЛ85’’’ sQT • -fy-P200.7+8.4 W634 O ; u’3?2'” • • • • , e • • .°V337 . • • • о • • U3613 -A- * M • 35 . * • • <38e < Ф • • 1.454 M+2-18-3 QV® • GEM Nl P204.1+4.7 Bi 8 RVo MONOCEROS Bill V742 ©• 06h52m ♦ • • • • • • • • • e 26 ’ • • • • • • • • • € • . <r • • Alhena _ <211 • • • • • •• • • • • • • • • • 23 • Christmas Tree Cluster 2264 • Cone Nebula. P201.7+2.5 2259 839 Hubble's Variable Nebula 2261 о I • 20 GEMINI • 0 •QQ.- MONOCEROS 837,38 □ 2247/- '•.♦□2245 +10° Bas 7 RW° Bas 8 2254 2. Plaskett s ' v640®tar ' 0106 Rosette Nebula 2237-39, 2246 • 2244 -----------® 06h36m )' Open Star Clusters and Asterisms Ч...7 to scale < S' Globular Star Clusters Ф® e to scale < S' Planetary Nebulae >30’ 30"-10’ 10"-5" <5" Bright & Dark Nebulae <2?O □°::: to scale 10 -5’ <5* Ge >s to scale laxies О О о 5’-2’ 2'-Г <Г major axis Galaxy Cluster ' " 4 \ J to scale 06h32m to 07h52m +18’ to +05° GEM CMI, MON W)j Пгюп / Barry Rappoport / Will Remoklui
96 Cone 06h40m +18° r 06h36™ 06h32m 06h28m 06h24m 06h20m Alhena ®W PI 94.2+2.5 . , GEMIN GEMINI* P201.7+2.5 +09° Hubble's Variable Nebula 0 2261 2251 / . Grill +05° 1-- 06h40m Bas 7f: 2254 ♦ 14 06h16m 1.2162 06h12m 0RI0N v/зк ©V1155 06h08m 06h04m УА}5Ь2-257 06h00m — , +18 © QQ, 2234 ф 72 f2 69 f1 19* ®PZ /Л' VI387 Sh2-261 . ©VI386 2224 ! ; 837,38—*^ 1.446 ; <12245 • Вы 8 1.448 • Cr95 /1.2169 2236 •. Plaskett's & V640^,ar * Crl06 ®AX 097 RS° ‘ , Д 3C158 ' У/ • & ° 1 t VI395 2169 67 V MONOCEROS VI392 ____о . M+J-/7- P204.8-3.5 2202 Skiff 10614.8+1252 2194 I VI388 . • .4 ©—*-------- . ,<>P/97.8-13 «Г 2141 Р198.6-6.3 +10 VI390 ° . P201.9-4.6 . VI389 —®— 2143 2186 Mt © “ . ® - 06h36m |V729 ;i2eJ ...................... J ) 06h28m / Rosette Nebula 2237-39, 2246 06h24m Stellar Magnitudes (V) andtx.9Mer 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 092 06h20m 06h16m 06h12m 06h08m 06h04m ORION . +05' 06h00m Double or Multiple Stars Individual members are plotted if separation exceeds 60" Variable Stars ф e ® @ @ ® (•) ® © Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag . Nova Q Quasar A Radio Source X X-Ray Source CopynghrC; 1987-2001 WiHmonn-M, Inc
др Open Star Clusters and Asterisms О О О to scale < 5' Globular Star Clusters ф ® Ф to scale < 5‘ Planetary Nebulae К/ -ф- -ф- < >30" ЗОМО" 10"-S" <5" Bright & Dark Nebulae □ n - to scale 10‘ - 5’ < S' Ga ^0 >5 to scale laxies О О о 5'2' 2’-Г <Г mapr axis Galaxy Cluster ( 4j to scale 05h20m to 06h40m +18° to +05° ORI MON, TAU, GEM Wit J тип i Burry Hupfjupurt I Witt Hcmoklui
97 05h28" + 18° г—. 05h24" 05h20m 05h16m 05h12m 05h08m 05h04m 05h00m 04h56m 04h52m + +( + 1 • +1( 1 +15 +14 • +13° • • +12° +11° • +10° - 115 111 17® • 7° (VII 9) • • • • • V1158 • . ° V1157 •- 03261 • • • • • • • • • • TAURUS « • V • •>’13 • . TAURI 5° -s-i • •no Q • . 3C138 JS • • • ...J • • • . 1817 Q1807 9 • • ♦ • • • • ° 03234 • • • • • •• • • • • • 16» ORION • • • • 0 ’e* • • ♦ • • • • • • • 15 • • • • 9 • • 111 © • • VI032) • • < 101 • • • V • ♦ 96 <• i060;; • • • ♦ • • _ Ф . • ♦ • • • 9 • • V1364 • * *• • -> V1361 • • ♦ • ♦ • 4 O' © • • • • • • • • ВVI057 vdB37 • • • ♦ • •- - • • • • • • • • ♦ • • • 9O2 • • Ф • • /663 () • • -♦ • ° • • ♦ • • ♦ • • • • • • • — «.— • • • • • • • • • • • • • • • • • -• DoDz 2 9 • • • >18 • • ♦ • — ♦ • • • • • • • 6g ♦ • • 1 1 I 4 \ x • % 1 1 ' B224 ♦ • • • • • • • •_ • -e • ♦ • • °. &-P190.. • • • -/7.7 • • • • • • • e 7 л1 1662 <J • • • +09° +08° - • • ♦ ♦ • — • • • • • • • • • • • • • • < 16 h • • • • 13 • • • • • • • • • • • < • • • • • • ♦ • 1 ♦ • • Do 19 - • • ° 032 vdB38/-\_ ’ ’ ” . V Lj; 8223 . — '93- • • • • • ♦ • • ° 03247 • ► 14 i • • • • • • - •. • • m a 1707 R- 03188 <•> ♦ • • o >2* * о 031724 03180 9 • 1-07° a • 06° — • *Do2? • • • Do 17 • • • • • • • M+l-14-9 -M+l-14-10 • < • • • • • • • • ♦ • * • • 9 • • • • ♦ C420-14 0 • • 1 n1 • Bellatrix 24 у • <=> 1875 • • ♦ 03282^ M+1- 4 03275 A539^W М+1-14-/ r. » 22 ч. U3269 74 ° M+1-14-3 • • • • • VI362 • • • • • • • • • • • • • • • • • • • 03181 • )5° !— • C421-30' M+l-14-36 ♦ • • • • 9 • M+l-14-3*, • А о • • • • • • 1819 • • • • • • A526 '' \ • x • _ 0 ui224 1 • .4 ✓ • • U3223 • • ♦ • • • о • • зл4 • • • • ORION * 05 28" 05П24^ 05^0" 05^16" 05^12" 054)8" 05*0 4m 05h00" 04h56" 04h52m 04h< • 0.0 Afxl bright • • • • N 0.5 1.0 1.5 2.0 Stellar Magnitudes (V) Г 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 I double or Multiple Stars individual members are plotted it separation exceeds 60" Variable Stars • © ® © © ® © ® ® (•) ® ° Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 maq. 4.0 maq. « Nova Q Quasar A Radio Source X X*Ray Source (.opytrghlC 1987-2001 Willmunn-tell. Inc. 04h48m * - 0 0 +16° +15° +14° +12° 0 +10° +09° +08° +07° +06° +05° Rm
9 04h08m — , +18° 041144m 041140m 04h48m +18° --- • • U3129Z • • • • IJ . • ♦ • • • • TAURUS ORION ] • • 92 ( 91 • r • O'* ♦ • • • • • • • • • • • • • • • • • e ► 93 04hl 2m 04hl 6m 04h36m 04h20m 04h32m 04h28m 04h24m 68 5s 3C114 61 5’ 64 S2 ’ n U2968 ° U3089 • 55 Aldebaran 87 a 75 H у 0 d e s 89 +16° ♦70 71 54 у ♦ 48 58 +14° +09°. +08 oV906 • 63 °V818 + 15° +07° 85 60 B3 79 b 90 c 1662 R« + 10° 66 r +09° C419-15 <=> U3067 +08° 46 о 1590 V1148 ДЗС/06 VI152 ”U3068 45 BIV Tau U3010 TAURUS 044 2m 04h16m 04h20m 04h24m 04h44m 04h28m 04h40m 04h36m 04h32m 1517 0 о V1151 • < U3061 ° U3066 +07° +06° C419-171 U3087 (3C 120) *®V1145 1633 I 1634 . ^U3122 ‘ - - +05° 04h08m +05° 04h48m + 12° +06° YU3172 RX • 86 p U3084 © 88 d C419-20 ЛП50 ^M+1-12'10' 81 << 78 80 ® 84 (VI146) . • 76 ф 73 7t 4Ы4.11 U2984 3C1O9 ® VI144 •®V1143 U2997A vdB26 47 M+l-12-4^ * 0 • • U3035' Wrf Tirion / Bariy Roppapuit / WiN Remokkn
98 04h16m 04h12m 04h08m 04h04m 04h00m 03h56m 03h52m 03h48m 03h44m 03h40m 03h36rJ + 18 !-----------------।----------------т----------------,--------------—---------------- +1 TAURUS 7° • • ♦ _ *0 1 • • • < 12968 • • • • . V471 • • • • 0 1.1977 9 9 • ♦ • +1 • • • • • • • • о • U2904 — — 9 • ♦ • < • • • • ♦ • ♦ • +1 +1( 5° Г • • • • • • +15 I • <48 0 9 • < • - — • • • • 9 V1131 • • U2894 • • • • • • • 0 [32823 9 9 *o 1384 • ♦ * +1 + 14 • • 9 • • * Л 4C+/4J1 • • • • • • • • ♦ ♦ • • • ♦ • • • • • • • • • +1 +13° 0 U2984 • • • • • • • • • • • • • ♦ • • • ♦ • • • V766 о № • q U2862 871 • • • • • • ЗС90д +1 +12° • • • • • • • — 0 • 9 • 5X ♦ • V1128 • • • • • • V1127 • 9 • +1 • •—1 +1 •a +1Г 3C109 • A • • __ • . • 9 9 ♦ - ♦ V1132 0 • ♦ • о ♦ • V1129® • • • 30e* - • +1 • vdB26 a • ©• • • 0357+107® 9 9 9 ♦ 3C98 A • 0 1.2002 • • • • • • 9 • +10° —•— — • 9 • • • 9 • • ♦ , 1 • ♦ • • • • • CH • • • • • + 1 +09° -9 47 • • • 9 • о • • • • A • • 9 49 p • • • • • +1 c ( +08° • • 12997 0 1517 л • • • • • — L • • • 0 • • • • • • • ♦ • • • U2829 0 9 • * +07° - <46 • • • • • a 3CI06 • ♦ • • • • • oX • • • • • ♦ • • • 9 • +1 • +06° ‘ M+/-JM4 ► • • • • 0 M+l-11-11 • • • • 38 V M+/-1 1-3 ^U2914 И+1-11-4 • 1462 , • 31 • • • 29 u • • • -M+l-10-8 • • • +( • ♦ +05°/— • • • — • • • *45 • 40 (V1133) • ♦ • • • • • • 9 °- _ A 4C+05.16 9 U2852 ♦ • • 9 9 3C93 * • TAURUS +1 1 xf —~~1-----•— —1-- ' 1---—'* t?"' —*- —1 +C 04h08m 04h04m 04h00m 03h56m 03h52m 03h48m 03h44™ 03h40m 03ь36а Stellar Magnitudes (V) mdXie- 0 5 1.0 15 2.0 2 5 5 0 5 5 4 0 4 5 SO 5 5 6 0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted if separation exceeds 60’ Variable Stars О ® @ <s> © (•) ® © ® ® ° Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. = Nova Q Quasar A Radio Source X X-Ray Source Copyright <t> 198 S-2001 Willmonn Bell. Inc
0 +18 +17 +16° +15° +14° • • +13° e • +12° 3h36m 03h32m 03h28m 03h24m 03h20m 03h16m 03h12m 03h08m 03h04m 03h00m 02h56 — • - 4 m 18° • Vl"l23 • TAURUS • • • U2716 ♦ U2684 t a • • • • • • • A3C79 • 53 M+3-9-1 ’<p<> Sc/Wc • ъ 50 U2486 • U2498 * • 46 p ♦ 0 U2424 ♦ +17° +16° 413 r t +15’ +14° +13° +12’ • • • • • • C464-14, • • > A 0316+162 • о • . U2602 • • • • • A 3C76.1 • U245 M+3-8-35 . M+3-8-36 ; л ° • • • • • • ?M+2 • • • -9-2 ’ •— • • • • / М+2-8-45 о U 2 ^7\M;3-8-32,, • • • V1122 0 • • • • • • • • • • 0 U2703 • • • • • .u • • • • • • • • • • ♦ • • • • ♦ • • • •• 5f M+2-< M+2-< 1 1 Oo V • ♦ • • • • • • • • • • • • • • • • • • • • -st • —• • • • • • • • • • • • • M+ • • • 2-8-48 0 • \ 7A401 U2438 —J A399 ’ +11’ +10’ +09° - • • • 4 s®’ ♦ V1120’ • < • • • • C441-2 • • AQ • 1168 0o1 • • M 66 U2437 +2-8-41 13^- +11’ J +10° I +09° • • • ♦ • • ARIES • • • 0 • 1236 X о • • • U2430 .* • a. M+2-8-37 • • 6te • • ♦ • °U2674 U2622 • • • 3- • • • • • • j 1.1873 ♦ 1.1862 • +08° - • • • 1 0 0 • • • • ♦ ♦ • • 1 .• • • • • • • ♦ • • 9 • 91 X . U2434 о J +08’ 9 J +07° • L132405 \U2399 •? J 1+06’ 40 1 A400 ✓ • - +05’ +07° - +06° - • • • • • • о U2740 • • -r—— 0 U2695 • • • • • • • ♦ • • ф • • _♦ • U241 0 44 8-27 • ♦ • • • • U2712 • • • • ♦ EL® • • • • • M+l:8-41 M+1-8-3 • * C41 • M+1-8 . M+l-8-j 3* °,-- • /\U24 5,.50.o M+1- •j4 । a • +05° • • • • -J. 1956 • • • • 0 • • • • TAURUS '-4C+05.14 CETUS • • • • • 0 M+1-8-4C • • • — M+1-8-35 ’ . U2469 ' M 9 Л C415- \ M+1-8-28 +1-8-36 U242t O3h3( >m 03h32m 03h28m 03h24m O3h2Om * 03h16m 03h12m 03h08m 03h04m 03h00m 02h56m Open Star Clusters and Asterisms j to scale < 5' Globular Star Clusters ф Ф- Ф to scale < 5' Planetary Nebulae >30’ 30--10’ 10’-5" <5" Bright & Dark Nebuiae □ ° ° to scale 10'-S' <5‘ Galaxies О О о о >5' 5-2* 2-Г <1* to scale major axis ca'“yau’“ 02h56m to 04h16m A +18° to+05° TAU ARI, CET Wi/ Ttnon / Barry Rappoport / Will Remakkn
99 03h04"i + 18° — 03h00m о 50 U2486 U2498 + 17° д 3C76.1 //o' 02h56m 46 p 0 U2424 M+3-8-35 •44 46° 02h52m U2303 02h48m 02h44m 36» 02h40m ---£__ 02h36m, 02h32m 02h28m 42 71 M+3-8-11 5 DoDz 1 4j° M+3-8-6 O AM о 1.248 Трозо M+3-7-40 02h24m । 1 Qo *27 ARIES +17° \M+3-7-49 . M+3-7-50 0235+164 M+3-8-29 + 16° .TW +16° 0 M+3-8-27 M+2-7-5 +15° 29 40* + 14° + 10° U2369 M+3-7-8 U2339 -S-o— U2329 о U2387 AN • о U1946 о M+3-8-7 ° M+2-8-31 U2378 , 1088 О 1168 f1166 M+2-8-20 1127^ | 11 ^0^2362 ‘1117 о 1.267 U2453^t36 U2437 М+2-8-41 о M+2-8-S °° U2252 37 0 о AG о 1.238 U1897 о 927 .1817 87 p U2007 1.1867 ® EG 1028 n n 1fr)A 1029 &° 1024 1.1846 ° U2238 U2041o 0 975 „1.1873 M+2-7-12 c^2-7-W .°^U1966 • A397 M+2-8-45 43 0 +15° 1.1857 +14° A397^M+^'^~^1 ' о U2282 J2348 /А401 о M+2-8-26 U2438 A399 M+2-8-48 [109 0 1111-1— 0 M+2-8-14 38 . U1883 0 + 11° ARIES CETUS U2430 - .... M+2-8-37 . U1879 +09° 91 К 1.1865 849 EE - U2255 . U2434 +08° +07° M+1 -8-33 U2419 ♦ M+1 -8-30 о 0 U2405 +06° +05° 03h04m | • U2323 U2336 0 ° oll07 0 M+1-8-5 I * / ^U2444 м51-15з1°^ I, ' С41“° 'A400 U2372 *^U2399 U2364 a о -% M+1-8-11A 0 * I U2367 I U2285 ' M+1-8-28 -8-36 M+1-8-35 <=> . U2469 ' M+ U2426 C415-6” 03h00m 02h56m 02h52m 02h48m ° DT 1.1825 о 1044 ° M+1-7-20 1046 & • JU2167 998 1 ft Q 997 U2092 +08° M+1-7-25 C414-40 +07° U2021 DX® U20750 0 U2176 1026 о +06° M+l-7-13 ’ U1982 M+1-7-5^. C415-4 1070 78 V M+1-7-4 * CETUS +09° 02h44m 02h40m 02h36m 02h32m 02h28m —+05° 02h24m 48* P • О 990 s Stellar Magnitudes (V) jndSJU 0.5 1 0 1.5 2.0 2.5 5 0 3.5 4 0 4.5 5 0 5.5 60 6 5 7.0 7.5 8.0 8 5 9.0 9.5 9.7 Double or Multiple Stars Individual members are plotted it separation exceeds 60’ Variable Stars • ® ® ® ® (•) ® ® (•) © О Amplitude Amplitude Amplitude Amplitude 1.0 mag. or less 2.0 mag. 3.0 mag. 4.0 mag. « Nova N Quasar A Radio Source X X-Ray Source (.upynghtC 1987 2001 Wilhnunn 8dl. Inc
99 02h24m +18° 02h20m е М+3-7-5 . о М+3-7-6 02h12m С461В-70 ’ M+i’6'49 • I OU1814 M+3-7-1 । +16° 1.1794 +15° о 882 02h16m о 02h08m •UY о M+3-6-47 о М+3-6-42 о 1.213 U1659 .b U1622 U1684 M+2-6-45 02h04m 02h00m -----Г М+3-6-18 U1495 о U1531 01h56m 01h52m 01h48m 01h44m ---, +18° ъ U1742 • 19 ---T, U163 &77 871 & .&870 876 PISCES ARIES U1219 M+3-5-13 Ul 328 0 +16° 8 1.1748 _U1372 G711 °ZZ U1420 U1211 U1261 О 1.1755 UJ432 о • M+3-6-13 RY. о U1512 AL197_____ 792 о 786 о M+3-6-8 OUI614 . <^1.1774 4С+15.05 °U1496 0 о 1.1780 1.196 Q> 1.195 U1242 M+2-6-21 М+2-6-46 о ^820 U1817 . U1702 + 14° C438-40 • © 8 +12° +12° U1558 + 11 24(; ARIES +10° +09° +08° +06° U1312o U1322O 716 • U1271 о 677 675 +07° U1687 * О о М+2-6-40 ф о\.1775 *oU1584 U1593" ь8ю U1274 а U1260r. U1282* cU1450 774 Л----- U1468 781 821 1.154 ° M+2-6-9 • U1694 DD 1100 UZ® 64 M+1-6-20 +08° ъ Ul 368 1.1772 к 1.182 DE° U1587 U1803 A245 M+1-6-25 0 1.1776 +06° A246 OU1775 ° M+1-7-3 0 676 864 U1383 __£1— U1237 М+1-7-5 о М+1-6-60 о U1669 о U1239 U1505 о М+1-5-47 0 М+1-6-18 U1290 О 683 673 : :^7 °U1605 ° М+1-6-30 +09° +10° +07° о 1,749 ' OU1395 1.156 о 665 • о М+2-5-24 . ° U1545 *1 М+1-7-4 572 7Г о 706 о 693 U1498 7£6 G I о 1.1770 --S— 1.1771 U1427 _ ___а___ U1425 0° м^-6'9 о о 742,741 М+1-6-23 U1435 М+1-6-24 ь Ul773 —с—г М+2-6-50 1.1791 1.222 CETUS 3C64 Ul 724 о 1.214 827 QU1663 U1670 M+2-6-22 U1580 1.193 N C438-2 U1391 1.202 1.199 c>U1649 .§1208 844 • 825 . ’ ^831 +05° L 02h24m U1646 G PISCES 02h20m 02h16m 02h12m 02h08m 02h04m 02h00m 01h56m • • о671 • • • • U1246 о ? М+2-5- OU1253 • • U1245 0‘. а • А. ' Ч6? М+2-5-39'U61 1/1326 *1/1325 01h52m ---— 01h48m M+1-5-33 —; +05° 01h44m о ъ 817 о U о 840 ’ Open Star Clusters and Asterisms k.,-: to scale < 5' Globular Star Clusters ф Ф ® to scale < 5' Planetary Nebulae <> -Ф- < < >30" 30е-10" 10"-5" <5" Bright ft Dark Nebulae n °::: to scale 10'-S' <5* Ge ^0 >s to scale ilaxies О О о 5' 2- 2' Г <1' major axis Galaxy Cluster to scale 01h44m to 03h04m +18° to +05° ARI CET, PSC WH Гтоп / Яапу Яаррароп / ИМ tonaklut
100 01h52m оо 01h48m 01h44m 01h40m ж о 777 7° & Ш328 4 + 16° + 15° U1219 М+3-5-13^. Г U1242 01h36m ♦ 103 • 105 . qU1176 628 M 74 M+2-5-8 • 101 01h32m U1093 Ю • U1113 о U1119 ^1.1711 01h28m €459-64 U1056 99 Г| AN О___ U1020 01h24m • 92 • M+3-4-34 О ’’ 1.1702 и?5.8 ---о----- €459-55 . 1.1700 №,10^ U 704 1 1698 О U985 01h20m qU903 ^U883 •?473 ’ О 463 476 _О_|------- U910 "U897 М+2-4-29 ° * ^933 01 h16m 01h12m — +18° PISCES .459 * oM+3-4-13 A171 А154 U 751 i 0 A158 C459-16 • 87 о U785 1.1645 A160 0 U838 ---------о— 475 0469 471 т * +15° C436-34 U1087 • 104 U1195 о U1083 +14° &3C49 U1211 @660 о U1026 U1110 ъ671 U824 . ’ ? U860 100 +12 о М+2-4-28 2 О: U1246 о • 0 U1057 М+2-4-22 ?U849 М+2-4-25 ° U1200 €436-16 о U774 М+2-5-18 и1209 о U1253 * U1274 о U1260 „ 01282ъ 0 U1290 о 683 0 U1245 673 U1312o U1322O 1 10 I + 12° 569 + 11° ARIES + 10° М/с oDD 110 О +09° +09° С) 1.1723 М+1-4-2 ° UZ® * U855 +08° oAQ о 638 • 96 +07° М+1-5-12 UV । А245 U882 U1239 4С+06.07 oCV U1014 98 Ц +06° — +06° М+1-5-4 e>U834 485 U803 „U1326 °U1325 ° 437 + 10° +07° +08° М+1-5-20 U1203 d 645 1.1721 ’ | % М+1-5-18 ' 1.162 PISCES ^1.161 м+2-5-39 0 0 631 М+1-5-8 М+1-4-27 ои№ I U1261 U1271 о 677^675 1.1715 102|7С оШ129 1.154 ' !56 о 665 о М+2-5-24 U1237 о U1206 °U1139 Ч U1144 +05° <-- 01 h52m U1191 о А240 652 А2464 106 V 0 676 U1167 о У 706 о 693 М+1-5-33 ЗС45 ---о— 01 h48m 01 h44m 01h40m 01h36m 01h32m Stellar Magnitudes (V) and brighter 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 9.7 U1024 _____ <^514 U1041 U1023 M+1 -4-60 U891 М+2-4-31 1.112 ъ U833 М+2-4-43 М+2-4-46 522 о 1.101 1114 . о525 ’ 524° ^5о^505 ’ ° ’ 509 532 518 .» о 489 з,. о 502 ^U808 1.1695 А193 U993 М+1-4-42 4C+08.06 A ♦ 95 01h28m Double or Multiple Stars Individual members are plotted if separation exceeds 60’ М+1-4-44 М+1-4-47 0 ° 0 U989 ©AR ^пп 492 486 500 490 • 0 488 о U887 01 h24m 01h20m 86 о М+1-4-^ eUY 88 М+1-4-7 €411-14 0 М+1-4-13 Л 455 ’ « •-LM+1-4-10 01h16m Variable Stars • © © ® (•)©© (?) ® О Amplitude Amplitude Amplitude Amplitude 1.0 mag or less 2.0 mag. 3.0 mag. 4.0 mag. ---1 +05° 01h12m и Nova Q Quasar A Radio Source X X-Ray Source Copyright © 1987 2001 Willmonn Bell. Inc
10< 0 + 18 1h12m 01h08m 01h04m 01h00m 00h56m 00h52m 00h48m 00h44m 00h40m 00h36m OOh32 • — - 4 m hi 8° +17° •+16° +15° +14° ) +17 J О C45 +16° r ' --'° 1 » 4 z +15° t +14° /1 ' 'iA154 • 4 _ z A13751 0 _ И+3-3-16 • • • • • • • • • U617 • • ♦ * • ♦ • ♦ U393 0 о M+3-2-19 • PISCES • • • '(4158 s / • « •** 9-16 ’ U708 C,U685 • • © • • • • • • • • • °M+3-3-8 • • • • • • 213 ° • • • • • •- 1.1645 1 • 4 60 • • ♦. > Pl 25.9-47.0 *0615 • • Q M+2-3-2 @57 • • • 53 AG U386 Л Q • • • U717 M+2-3-31 <72 о U677O • M+2-3-33 -M+2' • • ~22 U644 . Q • 0054+144 • 0572 • • • 533 • • • • • ° U488 • о M+2-3-3 • • • ♦ о 234 IW о T • 9 fk +13° » • +12° 1 r +11° +10° ? +09°. M+1-4-. о r • +08° . Uj27 'К o 1/722 >20 ф . • • ‘33 9 • • U627 о . ° 0100+130 9 9 • • • 0610 • ♦ • • • • • • • • 9 • * • • U385 о л 3C16 ’ • • • 1 • • +13° • +12° +11° • • • • • 75 • ♦ - c> о 0607 • . 0571 9 0545 о о М+2-3-12 о М+2-3-13 оСК ♦ • 0521 • • • • • • • • M+2-2-22 ol,31 • • • ♦ • • *1.62 oU603 • о 1.57 • М+2-3-7 0 1/500 58 • • 9 9 9 • • • • • • • • • • • • • 0 1.75 0 C435-40 • • • ♦ • 0 0558 • о/.53 • • • • • ЗС18Д- J.35 • • +10° • - +09° - +08° -2-26 r +07° >1 - +06° • • ♦ • • • & U63 9 ♦ • о U640 1 • • • • • ♦ ♦ • • • • • • • • • • „ J7422 • о‘Л ? ° U741 U706 . ° • • .0 • M+1-3-13 ‘ • • • • ♦ • о 0596 • • • ' 257* • С410-Г > • M+1°-2-54 • ^U418 • °180 9 • • • L M+1 -2-34 • • 1 ♦*£ +07° • • • +06° - 1 +os° ♦ • *70 71 e U634 • • 1.61 <?> M+1-3-8 • о 332 • • • О • U512 ° 1.55 • • • °250 • • 63 8 1 62 • • • M+1-2-36 < • • 190 ^-M+1-2-42 oM+1 » . • U335a aU331 • U705& • • • /л • • • • ©-WW • • • • • 60 240 • °. U429f 1.1569 ♦ • >1.1568 1.1566 ^1.1565 ' A76 • о • • • • • 80 e< • PISCES • 73 • • • • ♦ • • • • • ♦ V-..'/J592 J 0 Vo 1.1598 7 • > ’ -»C 1 • • • 410-2 /.1564 . • oU379 C409-37 о M+1-2-. 0 M+1-2-24 23 • — +05° 01h1. 2m 01h08m • 01h04m 01h00m 00h56m 00h52m 00h48m 00h44m 00h40m 00h36m 00h32m Open Star Clusters and Asterisms to scale < 5' Globular Star Clusters ф Ф Ф to scale < 5' Planetary Nebulae Bright & Dark Nebulae □ □ ° □ >30- 30"-10" 10"-5" <5- toscale 10'-5' <5' Gc >5' to scale laxies О О о 5 -2 2-Г < Г major axis Galaxy Cluster ; 'i to scale 00h32mto01h52,n psc +18° to+05° ari Wil Ttnon / Barry Rappoport I Wifi Remakk/ь
А1 — North America Nebula / Pelican Nebula (Chart 32) олг- 06 21h04m 21h02m 21h00m 20h58m 20h56m 20h54m 20h52m 20h50m 20h48m 20h46m 20h44m 20h42m т +47°00' +43°00' VI395 +46°30' +46°00 +46°00' +45°30’ +45°00' +44°30 +44c00 +43°30' +45°30' V2136 Bar B350 . 6997 +44°30' +44°00' 56 +43°30' +42°30' 4-42°00' V2138 0 +4Г30' B353 <J996‘ North America Nebula T , 7000 ‘‘ B356 . V1898 . O-V2144 (V193 )60? X у 15. ’ • • • • • 1 • • • • AZ 55(vi661).e V2132 ® • VI981 CO Cr428 B355 •: CYGNUS H +46°30' +45°00 P V2141® VI794 ® LDN935 1 • c. РШ+1.(Г • \ Pelican Nebula • • • 1 1.5067,70 •a / • / • • \'^B349 • 1 • г• • • • • V2134® +42°30' • • I . • • • • 0 • • • • • • • • • • • >TX . • • i . • • • +42°00' . • : > • 7027 .. • г • *® . V1059 • • • • • • • • • • • • • < • • * • 1 +41°30' * • • • • • • • • • • ♦ . 7024 •1 —L- • • • • • • • • • • • e • • • • +4Г00' - • • 2YCNUS ♦ • • • —•- • • *•’ @YZ • • • • • • < •_ [ • • ♦.; 58 V 21h04m 21h02m 21 h00m 20h58m 20h56m 20h54m 20h52m 20h50m 20h48m 20h46m 20h44m +4Г00' 20h42m Stellar Magnitudes (V) 20 andbnqht" 2 5 3 0 3 5 4.0 4 5 50 5 5 60 6.5 7.0 7 5 8 0 8 5 90 9 5 100 10.5 110 11.5 hint* Open Star Clusters & Asterisms Ф Ф Globular Star Clusters Bright & Dark Nebulae Objects are plotted to scale if larger than 2.5' >2.5' to scale Galaxies Ooo 2.5-1' Г-0.5 <0.5 major axis Planetary Nebulae >60" <> < 10"-5" бО’-ЗО" <5- CYG Copyright ф 1487 200> Willmonn-Bell. Inc — ------------------------------------------------------------------------------- WH Tirion ' Burry Huppupmt / Well RemuUui
Gamma Cygni Region (Charts 32 / 48) — AJ Stellar Magnitudes (V) • •••••••• andbc?hter 2.5 3.0 3.5 4.0 4 5 50 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 10.0 10.5 11.0 11.5 (aimer Open Star Clusters & Asterisms Ф ф Globular Star Clusters Bright & Dark Nebulae Objects are plotted to scale if larger than 2.5 Galaxies Planetary Nebulae -A- ,6o- i0M0, (// 0 ° ° ° v < 10Ч- >2.5’ 2.5-Г 10.У <0 5 60’ 30’ x <5. to scale major axis т -v <• j IVa) Tirol / Barry CYG Rappoport / Wrjr Rernaklui Copyright C) 1987 2001 WiHnwnn Bfll. Inc
АЗ - Galaxy Clusters Abell 2197 / 2199 (Charts 35 / 51 / 50) 16h36m +42°00' ---- I6h34m 16h32m 16h30m 16h28m 16h26m 16h24m 16h22m +41°30' +41 °00' +40°30' +40°00' +39°30' 6195 + 39°00' +38°3O' +38°00' - 16h36m HERCULES —-о— U10459 M+7-34-14 0 M+7-34-12 M+7-3 U10430 M+7-34-35 о U10436 ° U10427 A2197 4-110 U10415 U10407 * 0 М+7-34-51 М+7-34-52 • М+7-34-90 ° 6174 М+7-34-82 ° ° о М+7-34-81 M+7-34-92 & '6184 \o 6138a 6173 М+7-34-89 t М+7-34-97---- 6175 M+7-34-J02 о U10429 М+7-34-104. 1.4610 ®UY 16h34m A2199 \ ®GN V 16h32m Stellar Magnitudes (V) arxi&^hir 2 5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 10.0 10.5 11.0 11.5 fanter 6/60 М+7-34-31 о М+7-34-39 6150 M+ 7-34 -4 7 М+7-34-62 М+7-34-61 М+7-34-75 о * M+7-34-33 О и 10420 0 I U10404 61668 6166 о ° 6/66С M+7-34-79 М+7-34-67 - 6166А 6158 М+7-34-45 . Z 7 „ „ М+7-34-44 гМ+7'34-43 • M+7-34-57 0 ’ М+7-34-36 М+7-34-37 о 16h30m 16h28m Open Star Clusters & Asterisms 16h20m - +42°00' +41°30' +41 °00' 6/45 ; o6N7^l 6146 M+7-34-27 0 M+7-34-28 U10381 \ М+7-34-26 DoDz 5 ^6141 U10367 U10362 OU10354 3U10357 U10349 o. М+7-34-2 +40°30' +40°00' М+7-34-19' ^M+7-34-10 М+7-34-16 * М+7-34-13 О • * М+7-34-18 HERCULES 16h26m Objects are plotted to scale if larger than 1.7' . CORONA BOREALIS M+7-34-15 6131 М+7-34-5 А° Cl 96-50 о • • • • 6 16h24m _0 М+6-36-36 -------- 16h22m +39°30' +39°00' +38°30' U10344 О — +38°00' 16h20m ф Ф Globular Star Clusters <2? 'C ' □ 2; Bright & Dark Nebulae Galaxies >1.7 1.7 0.6 0.6' 0.3' <0.3' to scale major axis Planetary Nebulae A >60- ч> jo- io- 10-.5- <> «0--30- <s. HER CRB Copyright CD f 987- 2001 Willtnann-Bell, Inc WH Ttncm / Йапу Rnppapon / Will Remaklus
Perseus Cluster, Abell 426 (Charts 43/60/61) — A4 03h28m +43°30' 03h26m 03h24m 03h22m 03h20m 03h18m 03h16m 03h14m 03h12m 03hl om +43°30' PERSEUS +43°00' +42°30' +42°00' +40°00' +41°00' ? U2730 U2640 ' 32 I U2655 +43°00’ U2614 U2723 U2700 +42°30' U2654 U2568 +42°0C +4ГЗС +41 °0 1.292 о U2708 28 (D • PERSEUS U2604 0 • M+7-7-71 ;i 1.316 1265 0 о 312 +41°30' H • U2733 0 > U2725 1293 0 1294 . M+7-7-70 • < -------1276Л' 1275 Perseus A . 1283 о 01282 o 1271 281 1277 1.1907 1 . 1270 1267 • 4U2673 U2742 1.320 • °U2717 +40°30' C541-11 1/2736 _ M+7-8-4 « Mi7-8-11 +39°30' 03h28m 03h26m 03h24m П264 •j U2698 о 02686 t/2689 A426 ' Perseus Cluster 03h22m 03h20m Stellar Magnitudes (V) • ••••••«*................................... andbrjhter 2.5 3.0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 10.0 10.5 11 0 11.5 tat* CopyitghtC> 198 7 2001 Wilhnonn Bell. Inc U2659 • • • • C540-62 1.301 U2618 • U2608 U2612 C540-79 ’ 0 1257 ’••1260 ^[259 о 1.310 • • 0 1250 • • • U2591 0 • •. *• • • • • • • • * 0 • C540-59. L U2617 1.309 °' 1.311 03h18m 03h16m 03h14m 1224 * 0 ’•> 1.293 03h12m 01.294 +40° +40c --- +39 03h10m Open Star Clusters & Asterisms ф ф Globular Star Clusters <2?<7/ □ Bright fc Dark Nebulae Objects are plotted to scale if larger than 1.7’ Galaxies о о о 1.7 -0.6 0 6-О У <0 3 major axis Planetary Nebulae Л- >60" -Ф- 30’-10" 10’-5" 60Ч°" <5- WH Trion / fiony Rappapoct / Will Remoklui
А5 — Galaxy Cluster Abell 779 (Chart 56) 09h28m +36°00' — 09h26m 09h24m 09h22m 09h20m 09h18m 09h16m 09h14m +35°3O' +35’00' +34°30' +34°00' + 33°3O' +33°00' +32°30' + 32W 09h28m L • • • • • • 1 EO MINOR • • 09hl 2m ---- +36°00' LYNX M+6-20-49 M+6-20-46 0) M+6-2 / -33 0 M+6-21-38 U5020 TM+6-21 -36 U4837 +35°30' 2840 +35°00’ U4988 +34°30' 40 a +34°00' A779 +33°30' M+6-21-18 +32°30’ CANCER LEO °00' * 2779^ -2778- 0 2780 M+6-20-48 2859 U5015 U5011 M+6-21-32 M+6-21-29 04974 \ M+6-21-24 о 2839 е* 0 U4972 LYNX U4926 0 2823 -IX- 2833 1 2828 й 0 2827 ^2830 ’ t o 2825 2834 . 2829 02826 M+6-21-5 M+6-21-12 2793 +32°00' 09h26m 09h24m 09h22m 09h20m 09h1 8m 09h16m 09h14m 09h12m Stellar Magnitudes (V) ШЬфм 2.5 3.0 3.5 4.0 4 5 5.0 5.5 6.0 6 5 70 7.5 80 8 5 9.0 9.5 100 10.5 11.0 11.5 binw Open Star Clusters & Asterisms ф Ф Globular Star Clusters <2? О □ -7; Bright & Dark Nebulae Objects are plotted to scale if larger than 1.7’ >1.7’ to scale (.opynght © 198/-2001 Willmann-Betl, Inc. Galaxies о о о 1.7’ 0.6’ 0.6’-0.3’ <0.3- ma)Of axis Planetary Nebulae .« О LYN 10--5’ 6040* a <s. LMI, CNC Wtl Tinon / Barry Rappoport / Will Remaklut
Galaxy Cluster Abell 262 (Charts 62/61) — Ai Stellar Magnitudes (V) 7 0 7 5 8.0 8.5 9.0 9.5 10.0 10.5 11.0 11.5 • Open Star Clusters & Asterisms ф Ф Globular Star Clusters C?<7»z □ i’; Bright & Dark Nebulae Objects are plotted to scale if larger than 1.7' Galaxies Planetary Nebulae >1.7’ 1.7'06' 0.6' 0.3' <o.r to scale major axis AND TRI 2.0 and brightei Copyright® 1987-2001 Witlmonn-Bell. Inc Wil Пгюп / ferry Rappoport/ Will RemoldPs
А7 — Galaxy Clusters in Andromeda / Pisces (Chart 62) 01h32m +35’30’ 07 h30m 01h28m 01h26m 01h24m 01 h22m +33°00' 01h16m +35’30' 01h20m TRI ANDROMEDA M+6-4-2 . ‘ U940 513o +33’30' U862 ° C502-43 1.1680 о 1.1677 494 01.1689 U937 OU901 +32’30’ ®cw +35°00' 579 0 +32°00' 0 1.1683 + 34°00' + 34°30' о 472 о 1.1675 U913 U878 U911 1.1687 . М+5-4-26 483 ^1.1679 C502-44 * ° 1.1673 О 1.1682 496 о 498 о 0495 501 499 QS03 S512 M+6-4-14i U1086 4C+32.06 57 TRI PISCES U1033 01h30m 01h28m 01h26m 5150 517 * 0 566 0 468 U959 U975 о 01 h18m 582 +31’30' L - 01h32m 561 U1045 Stellar Magnitudes (V) . 536< 542 0 C502-84 529 523 о 528 • • U987 M+5-4-59 М+5-4-55 О) M+5-4-48 508 'i 507 1.1690 0 504 01h24m 01h22m *ndb£hter 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9 5 10.0 105 11 0 11.5 Ып» Open Star Clusters & Asterisms ф Ф Globular Star Clusters <2?< -V □ u; Bright & Dark Nebulae Objects are plotted to scale if larger than 1.7* to scale о/.1666 01h20m Galaxies +35’00' +34’30’ +34’00’ . ANDROMEDA PISCES +33’30' •o • Andromeda II • 449 ^U841 О М+5-4-14 01 h18m Planetary Nebulae M+5-4-12 ООО 1.7 0.6 О.б’-ОТ <0.3’ major axis >60" 60’30" о 447 +33°00' 65 +32’30’ +32’00’ 1 +31’30' bihi6m PSC AND, TRI Wi Tirion / Barry Rappoport / Will Remaklus Copyright © 1987-2001 Wtllmann-Bell. Int.
Galaxy Clusters in Andromeda / Pisces (Chart 62) — A3 2.0 and brighter 2.5 Stellar Magnitudes (V) Open Star Clusters & Asterisms Ф Ф Globular Star Clusters Bright & Dark Nebulae Objects are plotted to scale if larger than 1.7 Galaxies ooo 1.7-0.6* 0.6*• 0 3 <0.3 major axis Planetary Nebulae PSC AND, TRI VW Tiaon / Barry Rappapaa I Will Remaktus 3 0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 7.0 7.5 8.0 8.5 9.0 9.5 10.0 10.5 11 0 11.5 faster
А8 — Coma Cluster, Abell 1656 (Charts 71 / 53) 13h06m +30° l3h04m 13h02m 13h00m 12h58m 12h56m 12h54m 12h52m +29° о +29° +28°30 +28°00' M+5-3M32 +27°30' +27°00' +26°30' +26°00' u • • )' • • • • • • • ° U8076 X 138025 4 4 X + COMA BERENICES • • • + ✓ z z z z • z ;.M+5-3J-727 z z / 4952 6 . 4949 F о M+5-31-106o • 4922 .о ' 0'843' . oL4088 ^1.842 • 0 M+5-31-4! • U8069 0 * X • X X X X X X X • • • Coma Cluster A1656 . s X X X X X X ' J * i • • • • • ©их • Q 1.3990 • • • • • • 4793 • • • X X X X X X X X X X X X X X X • • • • • • • \-.4944 '4943 ° 4934 4929 4927 М+^'-954896 , 4 ws0 4907^ <=>* 1.4045 1.4040 4886 4908-^ v 48891 4 • 881 r • >895 A 4860 4851 ^>4858 48839^865 4Л74 4873 4ЯА4 о i41B^4841A • 4848 • • -46 4828 о • • • 4961 о • ’ 4957 °4960 ° 4931 • • 4926A о • m°<№ m,0 tm° S 49230 л 4911 4919° & M+5-31-94 M- о P49.3 926 7 4867 VARS 72^? 4871 4856 4875 4869 5-31-74 0 4854 +881 * Cl60-73 o4853 M+5-31-37.4 0 • °4< 4840 ' Cl 60-40 842A^4839 °4824 • <=>4805 • • • 316 e • • • 4807A 3C222 $4807 • • 3 M+5-30-111O • • • 0 U8122 • • • *M+5-31 • ♦ ' '^с>М+5-31-23 -36 48428 • 4827 4819 £ 4798 13900 °* 0 4788 4789Aq • 4789й o М+5-30-Ю90 1 f t < / / / ! t . M+5-30-116 4787 ° t • r • — • X X X X X X X X • X X X • • 0 489 • • 2 о U8C 4859 • • . 0 • 0 0 4821 М+5-31-18 80 • • z z z z z z . / z / / / / U8013 / • • X * • • COMA BERENICES • ** •- • • 1.838 * о 0 4849 • e> . 1.835 • • • < z z z • • 9 832 • • 30°00’ °30' °00’ +28°30' +28°00' 31 +27°30' +27°00' +26°30' +26°00’ 13h06m 13h04m 13h02m 13h00m 12h58m 12h56m 12h52m Stellar Magnitudes (V) indict" 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6 5 7.0 7.5 8.0 8.5 9.0 9.5 10.0 10.5 11.0 11.5 tale । . Open Star Clusters & Asterisms ф Ф Globular Star Clusters C? <1? □ □ Bright & Dark Nebulae Objects are plotted to scale rf larger than 1.7’ Galaxies 0 ° ° ° >1.7 1.7-0 61 О б'-О.У <03‘ to scale major axis Planetary Nebulae -А. >бо- -0- 30‘ ’0' -ф- 10’-5" -ф- 6040“ <5. COM Copyright (D 1987-200) Willmann-Bell, Inc. Wil Tirion / Berry Hoppapon / Will Remaklui
Hercules Galaxy Cluster, A 2151 (Charts 69 / 88 / 87) — Al 16h12m 16hl Om +19’30 16h08m 16h06m 16h04m 16h02m 16h00m +19’00' +18’30' +18°00’ +17°30’ +17’00',' +16’30' +16’00' +15’30' —• • HERCULES • • • • • • • • • • • • • • • • • • • • 0 . М+3-41-33 0 • 6028 •• • • • SERPENS CAPUT • • • • • • о * • • • • • • • •m • • • • • • • • • • • 0U10121 • • • C108-165 • • • • • • • • 0 M+3-4M37 • • • RO • 6067 о • C70^ ✓ oU1019S__ '"'0^6055 ’ ' 6057 438 • • ч Д2757 • \ Hercules Galaxy Cluster • • С108-46 b • • • . • • • • • • • * • • • • • • / / t ! ’ / L 1 1 1 1 • V X \ X 6056 b ' о 6044 182 & 604 ЗА'' млп 18605?^ ^6045 ^6040 60 6050 6047 ^6041 A,L * 6042 ъ 1.1178 ’ \ X X \ X X X • • < 1 ! ! / ! ! 6030 е ф 5г • • • • • • • • • • • • • M+3-41-141 \ .0 • • • • 8 • X X X X X • X X , X • • • H7K z z s. • • • • / s / г • • b 6034 м+з-< 0 -- - • • • • • • 1-47 • • 1.1151 • • • • !. /А2159 ф q • 6073 °• • • • • .. • © z ' г f f t ! • • / • • • x • \ . M+3-41-83\*‘ • ?152 • • • С108-59 • • • л • • • •• • • • • • r 1 1 I 1 •Д U10204 \ 4 X • О 1 M+3-41-95 < ! / / C108-117 • о • • • 1У10144 о • М+3-41-6/ • Z Z Z Z ✓ / / • М+3-41-2 «з • о М-) Ш134 .Д2747 i х : X X X I X 9 3-41-28 • • 6 • • • SERPEh • • • IS CAPUT • a M+3-41-124 .. 9.U102 • • • • • 01 • / 010143° ; С108-81 • 0 X X • 1.1165 0 • X X X X 4 4 1 । ; । ! । : / ! / ; HERCULES Z Z ✓ • 1.1155 0 ♦ • • • • • • • • о о 6022 15h58m +19°3( +19°0C +18°3( +18°0 0 16h12m 16h10m 16h08m 16h06m 16h04m 16h02m 16h00m 15h58m Stellar Magnitudes (V) £••>>•••••••« ttdbri^er 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6 5 70 75 8.0 8.5 9.0 9.5 10.0 10.5 11.0 11.5 tow Open Star Clusters fc Asterisms ф ф Globular Star Clusters <2?<7/ П ; j Bright & Dark Nebulae Ob|ects are plotted to scale if larger than 1T Galaxies 0 ° ° ° >1.7 1.7-0.6 0 6-0У <0.У to scale major axis Planetary Nebulae -A- >60* <> ^-10* < 10*-5’ v 60- 30- <5. HER SER Copyright © 198 7-200 J Wittmann-Bell, Im Wd Itnon / Borry Roppaport / Will Remaklui
Al О — Galaxy Clusters in Coma Berenices / Leo (Chart 72) 12h10m +26’00' ---- 12h08m 12h06m 12h04rn 12h02m 12h00m 11h58m 11 h56m 11h54m llh52m 11 h50m +21’00’ +20’30' +20°00' ।--- 12hlOm •S M+4-28-92 M+4-29-32 d. +25’30' &U7157 3920 о +24’30' +24’00’ +22’30' +22’00’ 4000 3999 0 1.746 +25°00' +23°30' +21 °30' +23°00' . <=\U7115 M+4-29-37 39973993 LEO U6806 /.762O 1147+245 Q U7143 о__ 0 Ш4-29-38 +25°30' U6861 +25’00’ +24’30' +24’00' 3983 +23’30' +23’00' M+4-28- 2 +22’30’ C 128- 6 +21’30’ 3910 M+4-27-78 U6876 • 4093 U6821 COMA BERENICES U6881 LEO 4098 4095 4060 ‘ 4056 4032 0 —o-7 3943 U6976 • Ci о 1.742 3919 _ M+4-28-77 A <? 3940 o 3954 3947 0 3937 4091 с ^^4089 4092 ’ «М 4057 4°66 о 4061 "•"“^,21-00' 3929 ~^М+4-28-70 4084 COMA BERENICES U7 141 ° U7137 12h08m 4101ъ 0 U7040 M+4-29-13 M+4-28-123 M+4-29-4 M+4-29-2 о M+4-29-/2 4090 - 4086 ’ 40?6 4072 • | gM+3-31-29 12h06m 12h04m 12h02m Stellar Magnitudes (V) +26°00' 4018 о . }yy} 4022 о 4009. 3989 4011 402’° 4023 401S M+4-28-117 . M+4-28-116° ' M+4-28-115 12h00m 2.5 30 3.5 4.0 4.5 50 5.5 6.0 6.5 7.0 7.5 80 85 9.0 9.5 10.0 10.5 110 11.5 t»inw U6847 U6846 M+4-28-87 °* 0 • 3951 1.739 0 4002 4003 3946 _a_*. 39268 <^-39264 o. . 0 3925 +22’00' M+4-28-65 +20’30’ 11h58m 11h56m I1h54m 11h52m +20’00’ 11 h50m Open Star Clusters & Asterisms ф Ф Globular Star Clusters C?<1 ? □ : j Bright St Dark Nebulae Objects are plotted to scale if larger than 2.5' Galaxies Planetary Nebulae <►»« COM >60" to scale 2.5-1 I - 0.5’ <0.5’ major axis 60" 30" LEO Copyrtght © 1987-2001 Willmann-Bell, Inc Wil J mon / Валу Rappoport 7 Will Remaklui
Galaxy Cluster Abell 1367 (Chart 72) — Al 11h50m +22°00 11h48m 11 h46m 1lh44m 11 h42m 11 h40m +21 °30' +2Г00' +20°30’ +20°00' +19°30' +19°00’ +18°3O' +18°00’ LEO • • • • • • • Q> M+4-28-33 • • • • • • • • • <3910 • 0 C127-55 Ut • • 743 о ♦ 92 • • • • • • • • • 3883 0 г • • о М+4-28-48 • • ' A1367 К 4 4 • U6607 о U6609 о 934 M+3-30-115 ►/ / 1 i / t / s • ✓ ✓ 3884 q / / / • C97-7 U6725 о М+4-28-47 • U6719Q >‘о s • 0 • 3821 M+3-30-51 о 3840 3844 о М+3-30-5 \* 3805 • < M+4-28-29 X X \ \ \ &3816 \ 5 ’ 0 3787 • • • t i । । । • । । • • X I \ • • . о M ’ 3886 387. • . 3861^ 3851 М+3-30-94 3841 v- • - 3842 +3-30-98 ° i<£>3873 . M+3-‘ ’ О 3862 т b3857 OU6697 ^>3837 °-7j 1.2951 • I. 1 » 1 1 • 1 1 • 1 1 1 1 1 . 1 / 1 • • "У6625 • °C97-36 • • • * • • \ M+3-30-/08. \ • \ X X X X X X M+3-30-//3 X • ^>3868 ^ 3859 • 0 ^>3864 3867 • • • — • z z z 3834 ’ / f ! ! t / / / / / / • • • • • • • • • • • • • о 3827 • • • • • • • • • • ©FY • • • • • B M+3-3C о U6670 V • • FW® • 0 136687 • -49 • • • • LEO 11h38m +22°00' +2Г30' +21°00' +20°30' +20°00‘ +19°30 +19°00' +18°30' +18°00’ 11h50m 11h48m llh46m 11h44m 11h42m 11h40m 11 h38m Stellar Magnitudes (V) andi^htc. 2.5 3.0 3.5 4.0 4.5 5.0 5.5 60 6.5 7.0 7.5 80 8 5 90 9.5 10.0 105 11 0 11.5 fainter Open Star Clusters & Asterisms ф Ф Globular Star Clusters <2?Bright & Dark Nebulae Objects are plotted to scale if larger than 1.7' Galaxies ooo и’-О.б1 0.6' 0 3 <0.3 major axis Planetary Nebulae >60" Ф -ф- 10" 5" <> 60’ 30’ + <5. LEO Copyright Ci 1987-2001 Willmann-Bell, Inc. Wil Tinon / Harry Rappoport / Will Remakkjt
Virgo / Coma Galaxy Cluster (Charts 91 / 90) — A12 12h38m + 16°00' г- 12h36m 12h34m 12h32m 12h30m 12h28m 12h26m 12h24m 12h22m 12h20m +15°30' + 15°00' +14°30' + 14°00' + 1 3°3O' 4584 0 +1 3°00' + 12°30' +12°00' COMA BERENICES ^4540 о 1.3522 4548 M 91 4571 1.3583 ' 4569 M 90 1.3586 4579 M 58 +11°30' +11°00' + 10°30' +10°00’ 4564 VIRGO • 12h38m 1.3540 . 4531O 4552 M 89 1.3510 0 I 12h36m 1.3365 1.3313 Q4312 9 1.800 4302^298 Q 4516 * 1.3501 U7436,.. ^4523 Q 1.3486 4322 ' 4321 M 100 I'»’"’ Omi ^1.797 <24419 04377 C4501 M 88 1.3478 4447 4374 M 84 4406 M 86 1.3475 . 4388 1.3363 & 4440 1.3 127 ^1.3381 43 3 4371 © KM 4299 4294 4330 '*4458 §4461 4425 1.3476 О • o 1.3311 о 1.3393 1.3331 Q) 4413 1.3344 cj 4436 06? 0 4431 O’ 4421 4452 О 1.3457 О 4287 *1.3103 0 1.3413 1.3418 o 1.3358 _ 1.3356 (J 4477 4479 0 | 4435 The Eyes А А • "44868 о* 4506 4396 4379 1.3432 q 4474/-, 4468 о 4459 1.794 a О 4473 Markarian 's Chain ' 12h18m --- +16W 4328 - o 0 . /7834 +15°3O' 1.3392 —<Ут- +15°00’ +14°30' 4254 M 99 U7355 +14°00' +13°3O’ COMA BERENICES 1.3355 0 4402 VIRGO ’ I.3W9 4306c c 4305 4267 +13°00' 0 1.775 1.3258 о + 12°30' 1.3489 4551 °0 4550 4567 ’ >0 Siamese Twins 4568 4497 1.3481 1.3499 ~XT 4491 4528 0 1.3470 о 4503' 4486M87 Virg0A - ЛЛ7< . ' 0 4478 4476 •. c 4486A 1.3459 ® <5 4351 • 4352 ----Ci--- 1.3188 • 20 0 1.3468 +12°00' +11°30' 12h34m 12h32m Stellar Magnitudes (V) 4482° 21.3425 12h30m 12h28m andtajhtff 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 65 7.0 7.5 80 8 5 9.0 9.5 100 10.5 11.0 11.5 fainter Copyright © 198 7-2001 Willmann-Bell, Inc. ^ 1.3371 0^25 04320 &4390 1.3328 ^4380 12h26m 12h24m 12h22m 1215+113 Q ’ О 1.3107 +10°30’ +1Г00' 12h20m +10W 12h18m Open Star Clusters & Asterisms ф Ф Globular Star Clusters Bright & Dark Nebulae Objects are plotted to scale if larger than 2.5* >2.5' to scale Galaxies О о ° 2 S'-Г Г-0 5' <0 5- major axis Planetary Nebulae VIR >60’ COM Wil Tirion / Barry Rappoport / Will Remaklui
Common Names A Coddington’s Nebula IC 2574 GX 14 Andromeda Galaxy NGC 224 GX 30 Coma Cluster A1656 GXCL 71, A8 Andromeda 1 GX 62 Cone Nebula NGC 2264 BN 95 Andromeda II GX 62, A7 Copeland’s Septet 72 Andromeda III GX 45 Corona Cluster A 2065 GXCL 69,70 Anon Platais ОС 32 Crab Nebula NGC 1952 BN !! Ant Galaxy UGC 6046 GX 92 Crescent Nebula NGC 6888 BN 48, A2 Ant Nebula PN G331.7-1.0 PN 182,196 Antares Nebula IC 4606 BN 147 D Antennae NGC 4038 GX 150 Dark Doodad BN 209 Antlia Dwarf GX 151 Double Cluster NGC 884 ОС 29 Aquarius Dwarf MCG -2-53-3 GX 124 Draco Dwarf UGC10822 GX 21 Arp's Galaxy GX 24, 38 Dumbbell Nebula NGC 6853 PN 66 Autumnal Equinox TICK 111 E В Eagle Nebula IC 4703 BN 126 Barbon's Galaxy CGCG 497-42 GX 45 Egg Nebula PK 80-6.1 PN 47 Barnard’s Galaxy NGC 6822 GX 124,125 Eight-Burst Nebula NGC 3132 PN 169,186 Barnard’s Loop Sh2-276 BN 116 Einstein’s Cross 2237+030 QSO 102 Bear Paw Galaxy NGC 2537 GX 40 Eridanus Cluster GCL 156 Beehive (Praesepe) NGC 2632 ОС 74,75 Eskimo Nebula NGC 2392 PN 75 Blackeye Galaxy NGC 4826 GX 71 Eta Carinae Nebula NGC 3372 BN 199 Blinking Planetary NGC 6826 PN 33 Eyes, The NGC 4438 GX 91.A13 Blue Planetary NGC 3918 PN 98 Blue Snowball NGC 7662 PN 30 F Bode's Nebulae NGC 3031 GX 14 Filamentary Nebula NGC 6960 BN 47 Boomerang Nebula BN 198 Fish on the Platter В 144 DN 48 Box Nebula NGC 6309 PN 27 Flame, The NGC 2024 BN 116 Box, The 54,72 Flaming Star Nebula IC405 BN 59 Brocchi's Cluster (Coathanger) Cr 399 ОС 66 Footprint Nebula Mi 92 BN 48, 66 Bubble Nebula NGC 7635 BN 18 Fornax Dwarf ESO 356-4 GX 175 Bug Nebula NGC 6302 PN 164 Fornax Galaxy Cluster AS 373 GXCL 174 Burbidge Chain 158 Fourcade-Figueroa Galaxy ESO 270-17 GX 83,184 Butterfly Cluster NGC 6405 ОС 164, A20 Frosty Leo Nebula IRAS 09371+1212 BN 93 Butterfly Nebula PN G10.8+18.0 PN 127 BW Tauri UGC 3087 GX 97,117 G Galactic Center RAD 146 c Gemini Cluster A 568 GXCL 58 California Nebula NGC1499 BN 60 Ghost of Jupiter NGC 3242 PN 151 Campbell’s Hydrogen Star PN G64.7+5.0 PN 48 Great Hercules Cluster NGC 6205 GCL 50,51 Canali ОС 130,131 Grus Quartet 177 Cancer Cluster 75 Gum Nebula Gum 12 BN 187 Carafe Galaxy ESO 202-23 GX 189 Carina Dwarf Galaxy ESO 206-A20 GX 188 H Cassiopeia A R+X 18 Hardcastle Nebula MCG -5-31-39 GX 167 Cat's Eye Nebula NGC 6543 PN 10,11 Haufen A A151 GXCL 140 Cave Nebula Sh2-155 BN 8,18,19 Helix Galaxy NGC 2685 GX 26 Centaurus A NGC 5128 GX 184 Helix Nebula NGC 7293 PN 142 Centaurus Chain 167,184, A23 Hercules A 3C348 RAD 87,107 Centaurus Cluster A 3526 GXCL 184, A23 Hercules Galaxy Cluster A 2151 GXCL 69,88, A9 Christmas Tree Cluster NGC 2264 ОС 95 Hind’s Variable Nebula NGC 1554/55 BN 78 Circinus Galaxy ESO 97-13 GX 208 Horsehead Nebula В 33 DN 116 Coalsack DN 198, 209 Hourglass Nebula PN G307.5-4.9 PN 208 Cocoon Nebula IC 5146 BN 31 Kei / GX = Galaxy GC = Globular Cluster ON = -- Dark Nebula R + X = Radio + X-ray GXCL = Galaxy Cluster Star Cid = Star Cloud PN = = Planetary Nebula QSO = Quasi-stellar Object OC = Open Cluster BN - Bright Nebula RAD = Radio SNR = Supernova Remnant
Hubble Deep Field Hubble’s Variable Nebula Hyades Hydra 1 Cluster Hydra II Cluster NGC 2685 NGC 2261 A1060 A 732 GX BN GXCL GXCL 26 95,96 78, 97 151,A19 113,114 1 Integral Sign Galaxy UGC 3697 GX 15 Intergalactic Wanderer NGC 2419 GCL 57 J Jewi'l Box NGC 4755 ОС 198 К Keenan’s System 12, 23 Kemble's Cascade 6, 28 Kepler’s Star SN1604 SNR 146 Lagoon Nebula NGC 6523 BN 145,146, A17 Large Magellanic C loud ESO 56-115 GX 212, A24.A25 Leo A Cluster A1185 GXCL 73 Leo Cluster A1020 GXCL 92 Leo Triplet 92 Little Dumbbell NGC 650-51 PN 29, 44 Little Gem NGC 6818 PN 125 M Markarian's Chain 91.A13 MayaHs Object MCG +7-23-19 GX 38, 55 McLeish's Object ESO 105-26 GX 206 Medusa Nebula PN G205.1 + 14.2 PN 95 Mice, The NGC 4676A GX 53 Millisecond Pulsar 4C+21.53 RAD 66 Miniature Spiral NGC 3928 GX 38 Minkowski's Object NGC 54? GX 120, A16 N North America Nebula NGC 7000 BN 32, A1 North Celestial Pole TICK 1 North Ecliptic Pole TICK 10,11 North Galactic Pole TICK 71 Northern Coalsack 32 Nova Persei GK-N1901 BN 43 0 Omega (Swan) Nebula NGC 6618 BN 126 Omega Centauri NGC 5139 GCL 184 Orion Nebula NGC 1976 BN 116,136 Owl Nebula NGC 3587 PN 24 P Parrot's Head В 87 DN 163 Parsamyan 15 BN 115 Pazmino’s Cluster St 23 ОС 28 Pegasus Dwarf UGC12613 GX 81 Pegasus I Cluster 82 Pegasus II NGC 7499 GX 82 Pelican Nebula IC 5067 BN 32, A1 Perseus A NGC 1275 GX 43, A4 Perseus Cluster A 426 GXCL 43, A4 Phoenix Dwarf ESO 245-7 GX 191 Pinwheel Galaxy NGC 598 GX 62 Pipe Nebula LDN 1773 DN 146 Pleiades IC 2602 ОС 78, A12 Polarissima Australis NGC 2573 GX 220 Polarissima Borealis Pyxis Cluster NGC 3172 GX GCL 1 170 R Red Rectangle BN 136 Reinmuth 80 NGC 4517A GX 110,111 Reticulum GCL 202 Ring Nebula NGC 6720 PN 49 Rosette Nebula NGC 2237-9, 46 BN 95,96,115,116 Running Chicken Nebula IC 2948 BN 209 S Saturn Nebula NGC 7009 PN 123 Sculptor Dwarf ESO 351-30 GX 176 Sculptor Galaxy NGC 253 GX 158 Seashell Galaxy NGC 5291 GX 167, A18 Sextans A MCG-1-26-30 GX 112,113 Sextans В UGC 5373 GX 93,113 Seyfert’s Sextet 69 Siamese Twins NGC 4568 GX 90,91,A13 Sigma Ori ОС 116 Small Magellanic Cloud NGC 292 GX 204, A26 Snake Nebula В 72 DN 146 Sombrero Galaxy NGC 4594 GX 130,131 South Celestial Pole TICK 220 South Ecliptic Pole TICK 211,212, A24 South Galactic Pole TICK 158 Southern Pleiades IC 2602 ОС 209,210 Southern Solstice TICK 145,146, A17 Spindle Galaxy NGC 3115 GX 133 Stephan’s Quintet 46 Sunflower Galaxy NGC 5055 GX 37 T Tarantula Nebula NGC 2070 BN 212.A24.A25 Taurus A NGC1952 BN у J Taurus Dark Cloud В 22 DN 77,78 Tempel's Nebula (Merope Nebula) NGC1435 BN 78, М2 Toby Jug Nebula IC 2220 BN 200 Trapezium 116,136 Trifid Nebula NGC 6514 BN 145,146, A17 Tucana Dwarf GX 204, 205 Tycho’s Star R+X 8 U Ursa Major 1 Cluster A1377 GXCL 24 Ursa Major II Cluster A1132 GXCL 24,25 Ursa Minor Dwarf UGC 9749 GX 12 V Veil Nebula NGC 6992 BN 47 Vela Pulsar R+X 187 Vela Supernova Remnant Gum 12 BN 187 Vernal Equinox TICK 101 Virgo A NGC 4486 GX 91.A13 W Whirlpool Galaxy NGC 5194 GX 37 Wild Duck Cluster NGC 6705 ОС 125, A14 Wild's Triplet MCG -1-30-33 GX 111 Witch Head Nebula IC 2118 BN 137 Wolf-Lundmark-Melotte System MCG -3-1-15 GX 121 z Zwicky’s Triplet 34, 35
09h 08h 07h 2 06h 05h 04h 31 03h Uranometna Star Map 10h Uh 12h 13h 21 14h 15h 44 16h 1 7h 18h 19h 20h 21h 02h 0]h V 00h 23h 22h Stellar Magnitudes (V) ф • ♦ Double or Multiple Stars ® 0 О Variable Stars Open Star Clusters Globular Star Clusters Planetary Nebulae □ Bright Nebulae Galaxies 00 0 5 1 0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 Iran Q.O Qopynqnt О 198/-2001 Willmann-Bell, Inc Wii I mon / Bony Rappoport / WtU Remaklui
03h 02h 01h 00h 23h 22h 21h 20h 19h 18h 17h 23" 22h 21n Stellar Magnitudes (V) @ О О Double or Multiple Stars Variable Stars Open Star Clusters Globular Star Clusters Planetary Nebulae Bright Nebulae Galaxies 00 0.5 1.0 1.5 2.0 2.5 3.0 inan u о 3.5 4 0 4 5 5.0 5.5 6.0 6.5 Copyright Г 1987-2001 WUhnann M. 1гк ИЛ/ Гюли / Barry Rappoport I Will RernukJui
Uranometria Star Map 23* 22* 21* 20* 19* 18* 17* 16* 15* 14* 13* Stellar Magnitudes (V) I ф • ♦ Double or Multiple Stars ® 0 О Variable Stars Open Star Clusters ф Ф Globular Star Clusters 4- Planetary Nebulae □ Bright Nebulae о Galaxies 0.0 0 5 1 0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 man u.u Copynqht C 1987-2001 WiNnwmi Bell. Inc Wti Ttoon / Barry Rappoport / Win Remak
IV Uranometria Star Map 1]h 10h 09h l9h 18h 1 7h 16h i5h 14h 13h i2h +60° +50’ +50° +40’ +30° +60° +20° +30 14h Bright Nebulae Galaxies И61 Tinon / Batty foppapcvt / Will Rerrmklui Capyttyhi C 1987-2001 Willmann-BcU. Inc Open Star Clusters Globular Star Clusters Planetary Nebulae Double or Multiple Stars ® 0 О Variable Stars ZTo °° °-5 15h Stellar Magnitudes (V) +40’ +2(
Uranometria Star Map V +60 +50° +40° +30° +20° +10° URSA MINOR CAMELOPARDALIS DRACO M82 M81 78 Mizar AUR ♦ 24 Dubhe Alioth • 16 • 19 ♦36 • 21 26% Ml 06 AURIGA CANES VENATICI URSA MAJOR • 34 59 е • 56 • to •19 43 • • 61 GEMINI >46 Pollux LEO MINOR •40 K'< • 72 M44 Algieba •95 81* CANCER • 46 Regulus M67 VIRGO 19л COMA BERENICES M65 OO *73 M66 • 43 •42 Merak M108 о q f M97 + P / Ml 05,, M96 0 OM95 74 * M40 70*.. ?1 Ф Megrez Л *37 4*ek-. •92 ♦ 93 • 31 LYNX • м/09/^eY / Phad Stellar Magnitudes (V) @ О о 0.0 0.5 1 0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 ’ 5.0 5.5 6 0 6.5 than O.Q Double or Multiple Stars Variable Stars Open Star Clusters Globular Star Clusters Planetary Nebulae Bright Nebulae Galaxies Серинг © 1987- 2001 Wilimann-Bcll, Inc WH Titian ! Barry Rappapott/ WHI RemaUw.
VI Uranometria Star Map llh 10h 09h 08h 07h 06h 05h 04h 03h 02h 01h DRACO 42* Dubhe M82 CASSIOPEIA ;мюз CAMELOPARDALIS • 43 ♦ 16 URSA MAJOR • a • 36 • 18 •24 ♦16 ♦ 19 • 45 • 36 • 48 32 • PERSEUS Capella 16® LYNX 66 64 AURIGA • 63 ♦ 40 65 • CANCER • 70 M38 Castor M37 © RT ♦ 26 Pollux •44 • 76 ♦36 ♦103 5 M35 ♦ 132 •121 • (0 63 ♦ 108 Ю5 TAURUS ♦ 36 Hyades V#16_ GEMINI ♦ 104 Aldebaran • 68 71 ®58 ♦ 45 • 84 126* 122 • 69 Alhena ♦133 ORION 66 ♦ 46 • MONOCEROS CANIS MINOR 42* >0 Pleiades1"! ? M45 • 125 ♦ 118 •S^CEPHEUS зЦе^>1 Mirphak M36
Uranometria Star Map 07h 06h 05h VII 21h +60° +50° +40° +30’ +20° +10° 04h 03h 02h 01h OOh 23h 22h 03h 02h O1h Stellar Magnitudes (V) 1.0 1.5 20 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 Double or Multiple Stars Variable Stars Open Star Clusters Globular Star Clusters Planetary Nebulae □ о Bright Nebulae Galaxies Copyright О 1987-2001 Willmann-Bell. Ini WW I mon I Barry Rappoport / Will Rernuklui
VIII Uranometria Star Map 21h 00h 23h +20° -20° ANDROMEDA +30° ^♦28 £ •73 78 79 63 719 67 • 72< 64 * __ 63. a Alpheratz 60* • 56 • 69 • T Scheat 46 38 • 52 • 46 • Z 65* • 51 • 0 ♦ 47 • 87 .48 ♦75 Algenib 76- ‘74 43* 42* • 86 81 70® 66 Markab • a 39 45 • 41*<40 LACERTA 47 •39 CYGNUS 49 • 0 32 ♦ 16* I •I я1 48 12 17 PEGASUS I • 31 К 19* • 18 • • 25 28 20* 21 52 14 15* 31< 27 VULPECULA • 33 30 26 428 ‘ 29 M/5 •Ф w 9е ♦ 16 *15 •П £ 52 34 ♦ : • 82 ♦18 • 77 •80 Enif E e • 13 30 PISCES ♦ 44 • Л 28 !♦ o* 00° IO- 101 • 32 0® ЕР о 69 11 12 30* 12 AQUILA 47 е* 46 £ • V 124 : *18 M73 • 29 • I •30 21 Ot К -30° DELPHINUS 29 31. 32* ♦ 25 • 26 5 •r 4 • *17 . • :19 58____ * ®55 59 • ♦ 57 13 14. • X J6 • 15 -10° 37^ • 34 ♦ 35 41» *36 p, 82 5 6 EQUULEUS (!)• -26 84 •14 • 60 ♦ К 96 67 .♦O CETUS 37 141 86 ♦ 49 • t 19 PISCIS AUSTRINUS •3 • 9 T • I SCULPTOR • 6 160 GRUS 1 21h 22h 23h 00h M30 41®$ 33 30 s.’ 44 -.....Ill • • V 144 143 ♦ 24 e • v •♦K 19 22. e 25 • • • 21 К * 9 ♦ 2 •! 104 106e * 103 108 107 82 • X 83< 81 78* 9 • 94 ♦ 97 •70 74. T2< ♦T1 •56 50 • 5 AQUARIUS 77 61 • 53 38 4S42^19ei ФМ2 103 .20 . 2ltf 16» e15 44 ♦- 45 • 98 - 99. * 101* 100 •• Stellar Magnitudes (V) 88 89* • 66 • 68 !)• ^7293 142 47 • 35 • K ♦ E 36 • Ф • M72 • ffi .27 •z CAPRICORNUS *17 21 Fomalhaut SCR 0.0 0.5 1 0 1 5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 than 0.0 • ♦ Double or Multiple Stars @ О О Variable Stars ♦ « MICROSCOPIUM Open Star Clusters ф Ф Globular Star Clusters <> Planetary Nebulae □ Bright Nebulae о Galaxies Cupyrry/U ip 1987 2001 Willmann-Bell, Inc Wil Tinon / flany Rappoport / Wiff Remokk.
l9h 18h • 21 +30 +20° +10° 00° -10° -20° -30° Xo • l 68 n E •8 : CYGNUS HERCULES • 39 17< • 48 • 19 • 41 • 15 16 • 24 • 17 29 102 • n ♦ 18 ♦ T •29 -e !• Q Albireo. PISCIS AUST. 19.’7 .•17 X» 25» •22 Uranometria Star Map 21h 20h ’42 \29\* 25/ ♦ 47 35* 2/ 52’ ’ LYRA • X 89 .79 к -•i 18 101 • 93 ♦ 18 •V ♦ 13 66 22 68 59 ОС • 61 OPHIUCHUS ♦ • 0 63* M28 • CO ♦ 8 ©M55 18* 8 SCORPIUS M7 Y 19h 18h □ Bright Nebulae Galaxies Bnghier Ihan 0 0 57 56 72 •71 Open Star Clusters Globular Star Clusters Planetary Nebulae •113 •112 • 110 6 0 6.S 9 • * Double or Multiple Stars © О О Variable Stars , ,Г,- 9 £♦ ’ Kaus Australis 87 83 84*~ Copyrighi >Г 19Я7-2001 Willmann-Bell tnc. Wil Ttoan / Barry Rappapoa / W>tt Remaklui PEGASUS M/5,' •ЗЭ ж df I 49 ♦ 52 • 32» °T 31* •зз 72* VULPECULA 27 • 30» 26 ‘ • 28 .17 10 ♦16 .15 ♦18 EQUULEUS 20 21* 16» -15 12 AQUARIUS 37 33 j/ 35. 36* • 7 30 M73 14’ DELPHINUS • 71 70 • ‘ 69"*68 5 >3 • E ’•13 .14 f*M27 »12 e. 13 M7I 15> H’o.s •10 ♦2 • 66* SAGITTA «w$i M5Z Фу, ♦v2 ♦ 111 ’08 109 107 • 105 106 104 .♦99 • 0 •78 • 100 97 98. * 95 V. Я .46 ф. ‘ *x 28»\ JI* .. CO2 co’ Rasalhague Altair 58. AQUILA ’35 ®T| 45* • I • 42 64 •74 • V • 36 ♦ 21 ♦ 23 •24 !• *61 27 14 15.» 26 12 MU 60 106 &M14 • 20 £♦ M26 <5 SCUTUM • a SERPENS CAUDA 126 M72 211 ’19 •20 •61 •v Ml 7^ M18 Ml6 • l) P <n O* >0 <SK>- J 27 •X 200е •; M75 •17 •4 CAPRICORNUS ♦ a MICROSCOPIUM 21h Stellar Magnitudes (V) .57 .56 P J>43 M24 Wf'pt/c 53 .•51 Я >50.. 290c • X’ 60!> eCO • 59 62® 20h 5' *29 .33 • • 21 • 15« V2' .3o 28 * 14t , - •?«()’ M21 > 26* Ф.24 r M22 Nunki M8 (5 SAGITTARIUS V1017 W ФМ54 ®M70 ФМ69 58 * -52 51* 44 '246 43
Uranometria Star Map 16h 15h 18h 17h МВФ It 50 59 • 4-30° 99 +3 ♦ 53 E a 50 34 CO I 45 +20° 59 M16 c ♦ 61 ♦ 68 72 • £ • Izar 39» • 56 57 •51 SERPENS • CAUDA SCT ♦ к 5( • I •26 • 93 • 32 17 •71 • 47 43* 66 0 1 • a • 4 0 00° 109 Ф M 4 -10° 37 8 • 0 48 s a2’ 29- 10 -20° ♦24 12 23 •4 w V1017 •Y SCORPIUS -30c 27 M6 М69Ф CENTAURUS 15h 16h 17* 18h Stellar Magnitudes (V) Bright Nebulae Galaxies Open Star Clusters Globular Star Clusters Planetary Nebulae Double or Multiple Stars Variable Stars 16 SERPENS CAPUT 109* • 108 49 ее ♦5 • 18 109 • *106 °* LUPUS •21 28 ВЛеп O.o 0.5 1.0 1.5 2.0 2.5 3.0 3 5 4.0 4.5 5.0 5.5 6.0 6.5 man o.o 73 • 74 22 е a •W ФМ4 Antares e13 d« *12 22 E • Kaus Australis M7 Copyright it) 198 7- J WiHmann-tk'll. I tic W>l faiun I dairy Rappoport / Wil/ /temokius 60 • V1 108 : 107 • 0 • 78 • 105 ♦ 100 98» 97 102» 96- 101 68 • 95 89 87 83 84-** •79 HERCULES Rasalhague Y 61 •M M23 ;58 • ♦ .52 CORONA BOREALIS 0 '/X ’‘мГ7и M18 * M24 » Y® M25 16: 21* 15' 14 M21 I M2p_t?VX- SAGITTARIUS • 8 70 ♦ 73 • ♦ 41 63 60 ♦ 54 • 49 • 29 ♦ 0) 10* ? .16 ♦ I .Г • K V Tft Is V 1) • X : 45 • 43 47 40 a BOOTES • 31 45 .37 19 21 16 14 30* ФМ10 OPHIUCHUS ♦ V Sabik E> ♦3 VIRGO • 23 ФМ12 18 16 50 • 20 MJ07 : o< OJ CO* Vе 1° , & MS 110 • X* 11 : <•---------a. 44 51 • <• <o 260" [cliptic M80 • 0 •43 & 45 26, M/9 •25 36»-M • II • 11 • 16 106 [3 Graffias #47 к41 CD2-’ 8 ‘ • 42 30 • 0 LIBRA ^•••32 28 2i0 v 148 •>•36 V i/*59 :60 55«*54 .56 57 •58 HYDRA 51» 52
XI 13h 12h Uranometria Star Map 15h 14h -10° -20° H -30° +30° +20° +10° 00° +2 -li -2( — URSA MAJOR . 00 15h 14h 13h 12* Stellar Magnitudes (V) Double or Multiple Stars 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 man о и ® О О Variable Stars © Ф Open Star Clusters Globular Star Clusters Planetary Nebulae □ Bright Nebulae о Galaxies 3( Copyright 1987-7001 Willmann-Bell inr WH Tmon / Bony Rappoport / LVj/.1 Remokiu'.
Uranometria Star Map 10h 09h 12h llh +20° +10° +30° +3( +2( 00° -30° -10° -20° 00 10h 09h llh 12h • Stellar Magnitudes (V) • • • • • • • • • • • < ♦ Double or Multiple Stars ф Ф Open Star Clusters Globular Star Clusters D Bright Nebulae 0 о Variable Stars Planetary Nebulae ° Galaxies Brighter than 0.0 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 40 4.5 5.0 5.5 6.0 6.5 -Ф- ♦ Copyright С 1987 2001 Willmonn-Bell, Inc. VW Пппл / Barry Rappoport / Will
Uranometria Star Map 8 09h 08h XIII 07h 06h 20’ +30° +20° +10“ -10° -30° 00° 17 +20“ 113 +10“ 31 -10“ -30’ 07h 06h 09h 08h -20° +30’ 00“ Stellar Magnitudes (V) q Я 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 Double or Multiple Stars Variable Stars Open Star Clusters Globular Star Clusters Planetary Nebulae □ Bright Nebulae Galaxies Copyright C 1987 2001 Wtllmann Bell. Inc Wil Гюоп / Яппу Лпррараа / WJf Remakku
XIV Uranometria Star Map 06h 05h 04h 03h M38 PERSEUS M36 M37 +30’ 54 •11 13 • 26 39 •55 • ц/ 4ie 49 GEMINI ♦Ф 60 5 ♦ 52 ♦ X 64 11 ♦ 98 ARIES 36 95 ♦ 99 M Pleiades 8 35 ♦ 33 • 41 • 44 ♦53 ► .49 56 * 59 *• 22 Alnath P • 9.5 > 66 T •65 •125 • 118 • 121 ♦ 40 • 42 О ..... T* Ecliptic 129 126* 122 -U3 l2y* ................1.1.6.' 20 - 120J19 .130 1 45 P« Я ?71^^8 6*4 57 139 z • /<? ♦ 132 ®RT •X 19. 18<Ь-17 16* ♦ 14 AURIGA 55 56* 62 • MIS ; 1 ’6^* 7 . V • 8 -.. Ro e TRIANGULUM 12 ♦30 • V ♦103 -----------«0» □'*. .Vioe'-y 114 Ю9 Ю5* Л • 106 ’107 ♦ 104 72 a L id 37 39 *• *•(!) •43 +20° 60° 14 13’ 97 • v 15 11 •35 18 + 10° 16 • Я? Л3 00° IO -10е -30° 26 27 .33 •32 ♦13 •14 /72 '• • 69 •no u •38 e31 -20° ♦ 15 ¥♦•16 ;135*131 137:’•♦133 134 ф Bellatrix .о .О "--..Г ° 29 19 TAURUS 74 75 • 66 6* V K4 97 45 35 • • 81 CETUS 39 • 19 ♦ d) FORNAX • o X2 • к 03h 04h 05h 06h V 45 • • 40 M7S * ♦ У >23 33 • 51 Mintakax ORION 63 2244 • 66 116 Mirzam x1 ; ©♦ • Betelgeuse • •52 59 • • 56 *60 M78 MONOCEROS 2!.’ 154 CANIS MAJOR *S.54 Л-.Я • 38 • 45,42 M43.42** * • I •55 , Saiph ак 136 LEPUS 22 J 66 • 17 • Y<*12 V’ COLUMBA I <©RX • K • *0 • 8 Stellar Magnitudes (V) ^h‘e' 00 0.5 1.0 1.5 2 0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 than 0.0 Copyright Ci 98/-2OOI Willmonn Ml. Inc 83.>821 Hyades Aidton“e“«e*J • 76 'l ♦ф C7 r Г •6 • 9*3 Л1 * _88 62 CO ♦ 30 31 . ♦ 29 • 12 118 25 93 •63 • 64 ♦ 51 .'46 • O', 24 . ®5____. M77 84 75 • 32 30 ♦ 22 •17 21 •56 ,47 o2 I4 •Э53 •я •°.59 *•58 CAELUM ERIDANUS • a 54 V2 U*e Ф • ♦ Double or Multiple Stars © О О Variable Stars 20 157 Open Star Clusters ф Ф Globular Star Clusters -ф- -Ф- Planetary Nebulae □ Bright Nebulae о Galaxies Wd Teton / Burry Roppupoit / Will ЙсчпсМм
Uranometria Star Map XV 03h 02h 01h 00h ANDROMEDA 63* • 11 13 55 39 59* 56* 41 49. •60 52 • 64 ♦30 •• 66 •V ARIES •H 26 27 TAU < 98 +10° II18 -20 -30° • 21 • 8 •47 • 35 ♦33 : 97 • 14 15 -10° T ;65*> r—63 00° +30° Ната1ф a • K 21* 11 • 73 67. 64* 72 ♦ £♦ • 4 • 1) 67 7 • ♦75 87 ...,•86 I 70 • • Л 34 ♦ • 82 77 •80 О 64 26 СО ♦ 51 I • 67 CETUS 14- ♦ 8 Deneb Kaitos 57 48 ♦ 101> 99* 100 □ • SCULPTOR • я 00h 01h 02h 03h V ♦ 15 8 < 62 *60 50 • 49 • 16 15 ♦74 •76 41 *35 • *36 13 14* * 11 • 58 PISCES 31: । 32 1 ty. 78 79 PEGASUS 69» *77 •89 £ DO* * 80 73 44 -10е • 40 R ♦ • 24 • • *17 PERSEUS +20° 54 ( P 3^.53 Pe 45 *40 oz * jo ♦ К 93 a 12 10< 16 14 10: TRIANGULUM 78 •82 5 • 91 •68 : 65 ♦ „28 a £ Alpheratz 95 94 ERIDANUS FORNAX 1.0 1.5 2.0 2.5 3.0 3.5 4 0 4.5 5.0 5.5 6.0 6.5 Copyright C f 98/-200, ^/illmann 8e/l. Inc •15 •1 у :109 94 •> p •97 • у2 • ijp 4*’ • a *o 29 38 31 • 6 69 •19 -.L.... 60 Y2< 84 *75 • 81 80 ••77 • £♦ • 71 Stellar Magnitudes (V) 70 71 Mira ♦ co 105* M74 О 10T • О 87* ♦72 •75 1OO 33* . 29 . 26 ё*36 •П 55 54 .66 *59 64 ♦ 57* 53* 52 46 •Ф ♦ 47 48 43 ♦42 ♦ 44 61 .63 • 66 43 42 ♦ 38 • *34 . 39 25 ♦ 32 *10.28 27 • 56 • 20 21 47 • 46 ♦ ♦ Double or Multiple Stars ® О О Variable Stars j___ :10 •14 13 12 29 • K2 ♦♦к1 Open Star Clusters Ф © Globular Star Clusters <> < Planetary Nebulae 22. -19 25. • •21 ♦20 AQUARIUS 104 108 -‘TJ03 • 107 106 : I , I П Bright Nebulae о Galaxies Wrl Imuft/ Ви(/уИи(.>{.Ч11МП/ WiHRemaklu1.
XVI Uranometria Star Map 23h 22h 21h Stellar Magnitudes (V) • ••••••••** 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 tnan о о ф Ф ♦ Double or Multiple Stars ® о О Variable Stars Open Star Clusters Ф Ф Globular Star Clusters < > Planetary Nebulae Bright Nebulae Galaxies Wrf Г/пил / Buriy ftoppaprvt / Win Rffnakkt Copyright О 1987- 200I Willmann-Bell. 1гк.
Uranometria Star Map ]9h XVII 18h 17h -40° -60° 13h -20° -30° -50° 22h 21h 20h 19h 18h 17h 16h 15h 14h 23h • • • Stellar Magnitudes (V) • • • • • • • • • • • * Double or Multiple Stars О о © ® Open Star Clusters Globular Star Clusters ° Bright Nebulae Brighter than 0.0 00 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 ® 0 О Variable Stars -ф- -Ф- Planetary Nebulae ° Galaxies Copyright © 1987-2001 Willmann-Betl, Inc Wrf Tinion / Bony Rappoport/ Will Rernukkii
Uranometria Star Map 13h XVIII 15h 14h -10° -30° -40° -50° -60° -1C -20 -31 l9h 18h 17h ]6h 15h 14h 13h 12" 11h 10" Miaplacidus Stellar Magnitudes (V) В"9*1?' 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6 0 6 5 Hun 0.0 ф • • Double or Multiple Stars @ 0 О Variable Stars Open Star Clusters Globular Star Clusters Planetary Nebulae □ Bright Nebulae Galaxies CopyrightC 1987 SMI WiUmonn-MI. Inc И/if 77г<1н/ Bnny/tyjpo/хут/ Will Remakkn
Uranometria Star Map XIX 10h 09h Alphard VIRGO M48 SEXTANS >*19 • 26 MON CRATER • к HYDRA • 16 • 44 CORVUS ea PUPPIS PYXIS ANTILA • w z-e- Me 1.2391 w® ♦ П • e 3532 b^ab1 Aspidiske 3372 Avior CRUX CARINA Canopus 2516 4755 201 Miaplacidus P PICTOR Hadar MUSCA VOLANS CHAMAELEON • a MENSA 02070 LMC APUS CIRCINUS Gacrux Mimosa • 19 ♦ 18 CENTAURUS >D •>u me VELA Copyright L 1987-2001 Wtllmann-BeH. 1гк.
Uranometria Star Map 05h 07h 06h -10° -20° -30° -40° -50° -60° 01h 10h 09h 08h 07h 06h 05h 04h 03h 02h Copyright О 1987-JOO I Willmann-Bdl. Ini. Wtl Гтоп / Barry Паррароа / Will Remakhn
Uranometria Star Map XX Copynght C> 198 7-JOO I Willmann-Bfll, Inc
XXII Uranometria Star Map 02h 01h 00h 23h PHOENIX GRUS ERIDANUS Achernar HOROLOGIUM INDUS TUCANA 204 Peacock SMC e RETICULUM HYDRUS PAVO DORADO OCTANS 2070 MENSA LMC PICTOR ARA Atria APUS «• • a CHAMAELEON VOLANS 2516 Miaplacidus CIRCINUS I 0 Avior MUSCA NORMA CARINA Kent 1.2602 Hadar 1.2391 4755 LUPUS 3372 Mimosa 3532 VELA Cacrux CRUX CENTAURUS V744 TRIANGULUM K* AUSTRALE • m Stellar Magnitudes (V) ф • ♦ Double or Multiple Stars (•) О О Variable Stars Open Star Clusters Globular Star Clusters Planetary Nebulae Bright Nebulae Galaxies .ВЛел 0.0 0.5 1 0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 6.0 6.5 Copyright C I987- 2001 Wittmann Bell. Inc Wtl Tinon / Barry Rappupuft / WiW Remukhn