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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’
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CopyngM© 19Ц 7-2001 Witlmann-Bdl, Inc
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12
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&
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Stellar Magnitudes (V)
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Copyright © J987-200I Willmann-Bell. Inc
13
> A1412
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M+12-11-42
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Copyrighr^ 1987-2001 Willmann-Bell, Inc.
14
09h36m 09h28m
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В ® ® ® ® © (•) ® ® @ ® ®
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Amplitude Amplitude Amplitude Amplitude
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Individual members are plotted
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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
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6916
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1/2112
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20*48
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6939
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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°
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6796
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6798
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19h28m
19h36m
19h44m
19h52m
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20h00m
M+9-31'20
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VI762® 21
гМ+9-31'21
48
+62°
♦ • ♦ DRACC • • • • ) • •
• • • • • • • •
► • • • • • • •
6831 о ° 6829
... 4
CYGNUS
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' 6787
о 6750
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ф 1 • •
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1)11435
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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
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6608 V 6/92
66/7° 55'6607
66096597 °6594
• • •
• ♦ ♦ • • «
0 M+10-26-17 •- • • •
♦ • • CY । A2293 ( ) •
* * . > •
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Amplitude Amplitude
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6562
-6566
6532o
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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/ .
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.6510 С • • • 6464 U11028 . ^6489 • •
M+10-25-104
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• "6497 •
• • •
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• •
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0 UW
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о
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6299
17h44m
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. 6286
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: м^-28; ь
010644
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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
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58
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U10454
M+9-27-50
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• • • • • • • • 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
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+62°
+61°
+60°
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121 ’ •
+59°
13 6
+58°
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1
+5»°
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5894
1.1099
M+9-25-29
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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
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• -— — —— - 1 •
• • ♦ • • 3C323 * 1 . A 1 © •
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• ————-
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• • • • • • • 59 5965 % 5963 71|<7O 5969 °
• • • • • • M+9-26-18 0 • c • 0 U10013 • — • !3C322 A
* M+9-26-32 • • • • • • • • ' • \ !• • • 1
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5875
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M+9-25-36
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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
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M+9-23-51 n
М+9-23-52 о
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M+9-23-42
14h08m
Amplitude Amplitude Amplitude
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5477o
5471
5462
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—+—5458 5455
5451
5451
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5449
5447 .
5450
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Amplitude A Radio Source
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Stellar Magnitudes (V)
Double or Multiple Stars
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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°
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13h44m
13h52m
о
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+56°
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13h28m
----------
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M+10-20-19
M+10-20-23
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M+10-20-16
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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
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12h48n
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12h16m
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28
@ ® ® © ® ® ® ® ® ©
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VW fmon ! Barry Rappoport / Witt Remakkn
29
Stellar Magnitudes (V)
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IW hnon / Barry Rappoport! Will RemakJui
32
Copyright $ 1987 2001 WiUmann-Bell. Inc.
® ’ •
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Stellar Magnitudes (V)
Double or Multiple Stars
Variable Stars
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Q Quasar
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Individual members are plotted
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S ® ® © (•) ® ® (•) ® О
Amplitude Amplitude Amplitude Amplitude
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20h48m
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Variable Stars
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Amplitude Amplitude Amplitude Amplitude
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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
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М+7-26-15
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4490
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U7950
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М+9-21-46
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М+8-23-80
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4085
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4096
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17654
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М+8-21-42
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11h52m
11h48m
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Stellar Magnitudes (V)
52 VI
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U6266
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176805
U6489
М+7-24-10
1121+422
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3600
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11632m
11h28m
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Double or Multiple Stars
Variable Stars
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URSA MAJOR
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11h16m
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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
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U6162
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+49°
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U6227
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U6201
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M+8-20-38
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U6075
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1 U5953
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0
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M+9-18
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M+8-20-89
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0
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U6101
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М+8-20-77
U6135
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C241-74
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+48’
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U6125_____
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U6129
U6131
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U6076
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+41°° —
3406
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М+9-18-72
о
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0 М+8-20-32
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U5698
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M+7-22-25
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M+7-22-60
10h36m
URSA MAJOR
10h44m
10h48m
10h52m
10h56m
11l'00m
11 h04m
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U5754
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M+7-23-18
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M+7-23-10
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M+7-23-15
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M+8-20
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U56O5
M+8-20-31
M+8-20-24
M+8-20-22
M+8-20-18
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45(0
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M+7-20 ’ M+7-2 3°,03009 67 0-66 .300S 3008 -% 2998
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6 0 6 5 7 0 7.5 8.0 8 5
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Individual members are plotted
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09l’48rn
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? US 198
0
M+7-20-32
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M+7-20-2S
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09h36m
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M Nova
Q Quasar
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Copyright + 1987-2001 Willmann-Bdl, inc.
39
+48°
+47°
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Stellar Magnitudes (V)
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Double or Multiple Stars
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51
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53
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М+6-25-59О
06393 *
+34° --
М+6-25-6/ <
+33° I
+32°
131°
+30°
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+29° I-----------
11h24m 11h20m
Hh04m
Л М+7-23-19
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11h00m
49
06?2/
о (.2616
° 1.2617
о 1.2620
М+7-23-8
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10h44m
10h48m
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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
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1
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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
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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
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М+6-25-42
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М+5-26-37
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1/5984
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10h48m
10*52™
10h56m
11h04'
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11 h16m
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05885
о
М+5-27-49
о
063/4
о
М+5-26-2
о
U6198*
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о
О
М+5-26-51
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М+6-25-36
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10h40m
о (75936
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М+6-25-21
М+б-25-15
- 3545ДВ, с М+6-25-14
--------J------—
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О М+6-25-22
д ^252
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о
о
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М+6-25-8
М+5-27-5
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(76152
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М+5-26-47
: 05990
о
46 .
oUV
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3442
• о U5898
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М+6-24-22
3396
3395
3424 о
2 3413 I.
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(75934
55
10h40m 10h36m
+41
+38°
10h28m
10h32m
M+7-22-25 °
i A1035
+40°
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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 |
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•M+6-22-34
_________a.
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UU®«
U5623 •27 .
™ •bUS622
28
1.2577
M+5-25-10
TX
M+5-25-30
+29°
10h40m
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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’
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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.
________
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U4953O
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8 M+6-21-40
’. 05020
M+6-21-36^
• 2859
05015 о
05011°
M+6-22-12
_ \o
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M+6-22-61
2942
3099
20
0152-10
0946+301
151
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» 05074
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3032
10h00m
09h56m
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CANCER
09h52m
09h48m
U5364
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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
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M+6-21-64
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30213013 ъзооз
M+6-21-42
M+6-21-51^.6^ ’
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’ M+6-21-52
M+6-21-70
V
M+6-21-46
° 05282
i LEO
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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
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I 3067 0
M+5-24-5
M+5-23-17 .
3106
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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
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VW
о V406
о V459
OB
48 RT
Sh2-241
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V394
44 К
06h00ni
06h04m
06h08m
06h12m
06h16m
06h20m
06h24m
06h28m
06h32m
06h36m
+29
06h40m
06h40m
I 1 0
AURIGA • •
0
W487
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1 • • • • • • • • • • • • • • • • • • •
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• • • ♦ V452 © .— • • • • •
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• • • • 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
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+39°
+38°
+37°
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m
+30°
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+36°
v436
V442
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V419
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+34°
v43
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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
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Sh2-231
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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 *
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05h32m
Variable Stars
Amplitude Amplitude
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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
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AM
829
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+32°
+29°
+31°
RX
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V413
1852
+39°
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TX
' 1.2120
0
V417
+35°
+34°^
19
Be 17
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16
+29° —
05h20m •05h16m
Open Star Clusters
and Asterisms
to scale < 5*
• • ♦ • • • •
4892 о
3C125
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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
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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
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03h16"
02617
. 1.309
02659 •
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о
U2857
AB
1.311
M+7-8-17
M+6-8-27
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+38’
, U2837
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+39’
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• U2828 ♦
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02709
02685
V496
U2710
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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
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. 02706
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02623 o
8206
B205
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+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
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03h20m
03^1
03h04m
02h56m
02h52m
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02h44m
02277
PERSEUS
"V568
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1.311
° 02256
002185
1077A 10778
12
1233 q
+39°
02709
57
+38°
® 02543
02636
1.1900
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U266i e;
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•I 02698
02689 02686 . .
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02546
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20
16
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02328
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V574
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02221
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03h20m
M+5-8-2
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03h12m
03h08m
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Stellar Magnitudes (V)
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02392
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U2222 Г
• ♦ • • 1 * •
• • • • • • • 1ч24в1о- •
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21 LT
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Q Quasar
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Copynqhtf) 1987-2001 Willmann-Bell, Inc
61
/Tj 02h08m 02h04m 02h00™
02h40m 02h36m 02h32m 02h28m 02h24m 02h20m 02h16m 02 12 ----
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Wil Tmon ! terry Rappoport / Will Remaklus
62
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+32°
+29°
02h04m
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S2m 01h48m
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566
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TRIANGULUM
М+5-4-56
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Variable Stars
Amplitude Amplitude Amplitude
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01 h20m
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Individual members are plotted
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Copyright?) 1987-2001 WHImann-MI. Inc.
62
01 h20m
+41’ r—
+39°
+38’
+37°
00h40m
00h44m
00h56m
01h00m
01h04m
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+25°
+19°
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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
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U11722
U11717
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011683^
to scale
to scale
V403
U11676
M+3-54-2
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>30" 30"-10" 10"-5" <5"
7003
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V402
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U11653
U11643
M+3-53-1
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DELPHINUS
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Galaxies
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major axis
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20h36m to 22"04m
+30° to +17°
PEG
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И6/ lirvri / Burry RafjfjufWft / Will Remaklui
66
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20h36m
20h32m
20h28"’
20h24m
20h20m
20h16m
20h12m
20h08m
20h04m
20h00'
P69.6-3.9
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+27°
+26°
30
+25°
+24°
+21°
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+29°
Be 83
23
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16
28
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15
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20h20m
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1.4954/55 □
Ro 4
FG° 6940
---- +
• 6853 1
Stellar Magnitudes (V)
Variable Stars
S ® (•) ® ® (•) ® °
Amplitude Amplitude Amplitude Amplitude
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в Nova
Q Quasar
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00
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Double or Multiple Stars
Individual members are plotted
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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
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su
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6823
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19h20m
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О
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Mi 92 a I
6842
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V396
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10
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13 VZ
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• • • • • • •®>6p • •
• • • • • • • • ♦ •
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V840
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U
+ P56.4-0.9 ®
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VULPECULA
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+21°
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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°
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+24°
+23°
+21°
+20°
. +19°
U11070
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+29°
+27°
Cl 72-4
1127
6680
+22° -
1071
U1U94
105
о U11113
+230
• 97
AC
oV990
96
0
V973
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IQ
V992
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U11107
M+3-4 7 -10
0
6548
% 6549
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+21°
Uli 237 °
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6500
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6364
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17h40m
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Double or Multiple Stars
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1
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U10944
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1.1268
/7204-246 ♦
70
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M+3-45-26
. &
M+3-45-25
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6427
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U11017
6518
U11090 **
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U11042 •
M+4-42-22
0 •
89 (V441)
U11043 .
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025
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0
87
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96
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16h52m
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17h04m 17h00m62/4 16h56m
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62
70
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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
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Stellar Magnitudes (V)
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Copynqhl © 1W-2001 Wllnvnn-M. Inc
69
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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
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U3489
uo
8e 23
2163
VI391
20
®VI155
GEMINI
VI387
ORION
L •
05h56m
06h00m
06h04m
06h08m
06h12m
06h16m
06h20m
06h24m
06h36m
PV
----?
+24°
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06*32" 2234 06*28"
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U3447
о
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.<115-6
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• 44 К < • • • • • • • _j. J- ®V394 • • • • •
V395 • P183.8+5.5 • eV451 • • . °V450 • • • • • • • • • •
• • •• • • • • • • • ' ►
♦ P184.8 • • 3(154 Q ^4.4 • • . TU • ’’ -AA -•— — • • •
• - -• • • • < .
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139
. P184.6+0.6
+25° I-
3C162’
10
11 LU®'
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99
WYg
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18 V
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OU
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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
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7П .
2175.1
3C152
8227
Skiff 10619.3+1832
1.2162
Sh2-257
Galaxies
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2 1 <
major axis
RW^1_.-TAURUS- +23°
•4 •l40 ... - -o- -
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64
V1385
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+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
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VI385
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V1167
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88° .
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Ecliptic
Be 72
1996
Be 21
PI 84.0-2.1
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2026
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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°
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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
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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
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72
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65 K’
39
70°
69a
65е
V834
50(0
4-:
74 e
68 83
04h00m
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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“
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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
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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°
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+29°
+28°
a
62
V837
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о AR
о AT
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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
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Copyright C 1987-2001 Wamann-BeH, Inc.
М+3-4-47
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М+3-4-37
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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°
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фа +11° • • < • • • M+2-2-/3 • * u< -♦ • '60 &M+2-2-10 • • ♦ • • • 63 о ‘ • • ♦ <34 • • • • 1.1526
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• +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°
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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
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1.1472
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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
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16h48m
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1.1206
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U9964
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U9978
5960
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Variable Stars
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Amplitude Amplitude Amplitude Amplitude
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• • • / • • • • • • • 4 —z4 ',‘A2055 г 2052 ‘ ° M+1-39-10 .C49-21 ^42033 • С48.ц • • )0 • • • • о U9625 •
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1)9625
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14h32m
14h28m
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0 U9244
+06°
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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.
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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
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° 5293
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51)
1882 4 1.881
1)8452
+15°
1)8383
5125
U8385
о
• 5180
4C+11.45
Q
1)8425
о
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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
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o* 5222
5230
1.901
1)8563
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• 1.900
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U8575
5209 oo
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5235
ъ 5224
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U8569
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+05° -------
13h52m
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08657
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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
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о
U8322
С72-41
5058
5100
59 е
о 5080
VIRC0
5020
+16°
+15°
+14°
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* о С72-23
1)8298
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• 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
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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
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i.3W " °4639
4654 <?
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1.3611
о
1.3718
1.3720
о
34
4694
4620*
. °l.810
4640
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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
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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
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^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'
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^4551 о
«4550 l3489
, 1.3459
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Siamese
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4528
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• '\3499
1.3481
1.3470
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4578
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M+2-32-161
1.3617____
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U7802
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1.3518
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1.3517
о
20
’ 1.3468
.....H +10°
1.3487
Q4522
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л 4519A
4519 ।
4535
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07688
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C42-153 ’ 4Л 8
• 45188
4526
+08°
°4570 о.>Л/С1
R ОЦ7795 | 18521
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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
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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 •
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4421
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4312
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12h12m
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12h08m
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1.3638
+ 10°
+09°
4598 о
+08°
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1.3392
Л4501 М88
44'4<"Л
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4506
1.3501 о
4477
4479
44730
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099-16
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M+3-31-61
& 07074
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07100
12h04m 4048 12h00m
— ------j +18°
окм+з-31-15
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07327
о
о
4239
4237
4584
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4419
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4447
1.781
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4262
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1.3096
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4152
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M+3-31 -28
М+3-31-25
07032
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? 07196
6
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4254 М 99 1.3077
< 07355
о 1.3065
о 1.3023
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1.3091
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1.755
069-29 О
1.3019
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+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
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1.3303
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4528 13481
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4497 • О
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4578
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1.8468
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о
1.3371
1.3518
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о
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1.3170
4307
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1.3060 13036
1.3039 о
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0 4532
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12h36m
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1.3271 .
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4366
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1-3148 о o 1.3131
4276 . 4233
4224
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4334 .
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1.3259
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- 1.3218
4297
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1.3268
1.3225
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4333
^39о1р4826 4269
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4376
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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
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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
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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
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+15°
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0
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+09°
+08°
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+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
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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
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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’
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• ♦ • • • • 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
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99
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P •
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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
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+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_____
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о
786
о
M+3-6-8
OUI614 . <^1.1774
4С+15.05
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1.196
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8
+12°
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+ 11
24(;
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+09°
+08°
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716
•
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о
677 675
+07°
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ф о\.1775
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1100
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+08°
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1.1772
к 1.182
DE°
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0 1.1776
+06°
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0
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864
U1383
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о
М+1-6-60
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М+1-5-47
0 М+1-6-18
U1290
О 683
673 :
:^7
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° М+1-6-30
+09°
+10°
+07°
о 1,749
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1.156 о 665
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М+2-5-24 .
° U1545
*1
М+1-7-4
572 7Г
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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
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01h48m
01h44m
01h40m
ж
о 777
7° & Ш328
4
+ 16°
+ 15°
U1219
М+3-5-13^.
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01h36m
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• 105 .
qU1176
628 M 74
M+2-5-8
• 101
01h32m
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о
U1119
^1.1711
01h28m
€459-64
U1056
99 Г|
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U1020
01h24m
• 92
• M+3-4-34
О ’’
1.1702 и?5.8
---о-----
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1.1700 №,10^
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U985
01h20m
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463
476
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^933
01 h16m
01h12m
— +18°
PISCES
.459 *
oM+3-4-13
A171
А154
U 751 i
0
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C459-16
• 87
о
U785
1.1645
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0
U838
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475 0469
471 т *
+15°
C436-34
U1087
• 104
U1195
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+12
о
М+2-4-28
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U1057
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98 Ц
+06° —
+06°
М+1-5-4
e>U834
485
U803
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+ 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
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о
U1206
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+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'
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+12°00'
COMA BERENICES
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4569 M 90
1.3586
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+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
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1.3328
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12h24m
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+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
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05h
04h
31
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Uranometna Star Map
10h Uh
12h
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19h
20h
21h
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23h
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ф • ♦ Double or Multiple Stars
® 0 О Variable Stars
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Wii I mon / Bony Rappoport / WtU Remaklui
03h 02h 01h 00h 23h 22h 21h 20h 19h 18h 17h
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Stellar Magnitudes (V)
@ О О
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Variable Stars
Open Star Clusters
Globular Star Clusters
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Bright Nebulae
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ИЛ/ Гюли / Barry Rappoport I Will RernukJui
Uranometria Star Map
23* 22* 21* 20* 19* 18* 17* 16* 15* 14* 13*
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I
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VW Пппл / Barry Rappoport / Will
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Copyright C 1987 2001 Wtllmann Bell. Inc
Wil Гюоп / Яппу Лпррараа / WJf Remakku
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Copyright О 1987- 200I Willmann-Bell. 1гк.
Uranometria Star Map
]9h
XVII
18h
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Copyright © 1987-2001 Willmann-Betl, Inc
Wrf Tinion / Bony Rappoport/ Will Rernukkii
Uranometria Star Map
13h
XVIII
15h
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И/if 77г<1н/ Bnny/tyjpo/хут/ Will Remakkn
Uranometria Star Map
XIX
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Uranometria Star Map
05h
07h
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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
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PHOENIX
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Copyright C I987- 2001 Wittmann Bell. Inc
Wtl Tinon / Barry Rappupuft / WiW Remukhn