OF THE ROGER N. CLARK
OF THE ROGER N. CLARK
OF THE ROGER N. CLARK
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Appendix E<br />
A catalog of deep-sky objects<br />
This appendix lists the 611 deep-sky objects<br />
that, in the author's opinion, are the most<br />
interesting for amateur astronomers. The list<br />
represents a search of the literature for objects<br />
that are both interesting to observe and<br />
also have photographs widely available. I<br />
culled the information from many sources:<br />
Burnham's Celestial Handbook, magazines such<br />
as Sky & Telescope, Astronomy, and Deep Sky; Sky<br />
Catalog 2000.0 (Volume 2) , and professional<br />
journals such as the Astrophysical Journal.<br />
In compiling this catalog, the first step was<br />
to check that an object might be seen through<br />
average amateur telescopes. Then I searched<br />
for those that might show some features.<br />
Many objects within range of small telescopes<br />
were left out because they are so near<br />
the limits that most would just look like<br />
another fuzzy patch. The present list still has<br />
many of these (depending on your telescope<br />
size an sy quality), but many others clearly<br />
show slgmficant detail and have much text<br />
devoted to them in books like Burnham's.<br />
When going out for an observing session,<br />
one wants to know which objects will be visible<br />
that n .<br />
ight. Some books (e.g. Burnham's)<br />
are orgamzed alphabetically by constellation,<br />
so a search through the entire work is required<br />
in order to find out what there is to<br />
s <br />
e. This list, on the other hand, is ordered by<br />
nght ascension. For any given night, one can<br />
start at some point on the list and work<br />
downward.<br />
The following data are tabulated:<br />
ID: The NGC number of the object, or other<br />
atalog number if the object has no NGC<br />
:slgnation. The Messier number is also<br />
glv<br />
d<br />
en If appropriate. Before the ID several<br />
ax appear. An astensk (*) means the<br />
IS .<br />
Iscussed m the book and a drawing<br />
co es m . '<br />
obj ect '<br />
and<br />
Con: The constellation in which the object is<br />
located. The following standard abbrevia-<br />
tions are used:<br />
photograph are presented in Chapter 7.<br />
An S indicates the object is a star cluster with<br />
star magnitudes given in Appendix B. Exclamation<br />
points indicate the object is an<br />
es ecially fine-looking one, with four (!!!!)<br />
bemg the most spectacular visually.<br />
Positions: Positions in right ascension (RA)<br />
and declination (DEC) are tabulated fo r<br />
equinoxes 1950.0 and 2000.0. Both are given<br />
because star charts for both equinoxes are<br />
common. The RA is given in hours and de<br />
imal minutes of time, and the DEC is given<br />
m degrees and arc-minutes. The objects are<br />
sorted by increasing 1950.0 RA. The positions<br />
in the catalog have been checked<br />
a ainst se eral other catalogs, and as many<br />
discrepanCIes as possible have been eliminated.<br />
One good reference is Sky Catalog 2000.0,<br />
Vo lume 2, by Hirshfeld and Sinnott (1985).<br />
The 2000.0 positions in this list have all been<br />
che ed ag inst Hirshfeld and Sinnott. Many<br />
pOSitIOns disagree in the last digit between<br />
the two catalogs, but the differences are not<br />
significant and can be attributed to round-off<br />
error, or to where the exact center of a large<br />
object was chosen (a center may not be obvious<br />
in open clusters and nebulae in particular)<br />
. When the position disagreement was<br />
significant, I investigated and chose the best<br />
position. In some cases that meant measuring<br />
photographs. Several small galaxies in the<br />
c uple-o:-arc-minute size range had positions<br />
dlsagreemg by about an arc minute or two.<br />
However, the coordinates are always accur<br />
te enough to find an object with setting<br />
CI rcles or by plotting on star charts, even at<br />
.<br />
high power.<br />
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