| A |
component A of a double or multiple star |
|
adj |
adjacent |
|
B |
component B of a double or multiple star |
|
B |
(with number) Barnard's catalogue of dark nebula |
|
C |
component C of a multiple star |
|
CC |
concentration class for globular clusters, from I to XII |
|
Cl |
cluster(s) |
|
cn* |
central star of planetary nebula |
|
d |
degree |
|
Dbl |
double star |
|
dl |
dark lane in galaxy or emission nebula |
|
DN |
dark nebula |
|
EN |
emission nebula |
|
G |
galaxy (with type) |
|
GC |
globular cluster |
|
IC |
Index catalogue |
|
-in |
inch (as in "8-in", meaning a telescope of 8-inch aperture) |
|
inv |
involved |
|
LMC |
Large Magellanic Cloud |
|
M |
Messier catalogue |
|
m |
visual magnitude |
|
mag |
visual magnitude |
|
Mlt |
multiple star |
|
[name] |
the originator of a descriptive name |
|
NE |
visible with the unaided eye |
|
Neb |
nebula |
|
NGC |
New General Catalogue |
|
OC |
open cluster |
|
OIII |
An Oxygen III nebular filter is recommended |
|
p |
photographic magnitude |
|
PN |
planetary nebula |
|
Ri |
rich in stars |
|
RN |
reflection nebula |
|
SMC |
Small Magellanic Cloud |
|
SNR |
Supernova remnant |
|
st |
star(s) |
|
UHC |
A filter passing both OIII and Hydrogen Beta is recommended |
|
Var |
Variable Star |
|
? |
the author questions the NGC2000.0 visual magnitude |
Galaxies are identified by their Hubble type .