NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2018-07-21 T06:13:15 PDT
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Notes for object NGC 0922

7 note(s) found in NED.


1. 2006ApJS..165..307M
Re:HIPASS J0224-24
HIPASS J0224-24.This collisional ring galaxy system (Lynds & Toomre 1976;
Hernquist & Weil 1993) is similar to the Cartwheel galaxy (see e.g., Fosbury &
Hawarden 1977; Higdon 1995). The primary S1 (NGC 922) has a C-shaped morphology
and is the ELG with the highest H{alpha} luminosity (L_H{alpha}_ = 1.8 x 10^42^
ergs s^-1^) in SR1, while we identify the interloper S2 as the compact H{alpha}
bright galaxy 8.36" away to the WNW. Wong et al. (2005b) present a more detailed
analysis of this system using a variety of observations including the SINGG SR1
data.

2. 1994CAG1..B...0000S
Re:NGC 0922
SBc(s) pec
CD-1600-S/Br
Aug 12/13, 1980
103aO + GG385
45 min
The morphology of NGC 922 is so peculiar
as to be outside the classification system. It would
be called a sport by nineteenth-century animal
breeders. The reason for its inclusion in this
section is because it appears to have a central bar
from which spiral fragments are attached,
primarily on one side. These fragments spiral
outward at very large pitch angles, abruptly stopping
at an edge. HII regions exist throughout this
half of the image. The other half is devoid of
high-surface-brightness features, although
smooth, low-luminosity plumes exist there.
Two prints of NGC 922 are shown here. In
the heavy print above, the smooth, low-surface-brightness
features are easily seen. The light print
below, made from the same original plate,
shows well the HII-region candidates in the bar
and in the high-surface-brightness parts of the
image.
NGC 922 has no evident companion at the
same distance that can be blamed for the peculiar
morphology from a supposed close encounter.
The redshift of NGC 922 is v_o = 3061 km/s.
The absolute magnitude of the galaxy is bright at
M_B_ = -21.7.

3. 1985SGC...C...0000C
Re:NGC 0922
Plate 2708
Overexposed center and bar, dist arms with many knots. Faint plume to
north-preceding.
Plate 5522
Possible colliding pair with companion superposed?

4. 1982ESOU..C...0000L
Re:ESO 022248-2500.9
=ESO 478- G 28
numerous knots

5. 1976RC2...C...0000d
Re:NGC 0922
Possibly interacting with an anonymous SB(s)b: at 13 arcmin

6. 1974UGCA..C...0000N
Re:UGCA 030
UGCA 030:
= NGC 0922
SB(s)cd pec (RC1)
singular; blue, chaotic object with bright knotty spiral arc on following side;
extremely diffuse spiral arc on preceding side;
hints of short internal spiral arcs; eccentric nuclear region;
no regular transition case in Hubble's system;
paired with UGCA 032

7. 1964RC1...C...0000d
Re:NGC 0922
Bright nucleus in short narrow bar: 0.5 arcmin x 0.08 arcmin,
Several knotty filamentary arms.
Strongly asymmetric, hexagonal outline.
Pseudo (R): 1.3 arcmin x 1.1 arcmin.
Interacting pair (?) with anonymous SB(s)b: at 13 arcmin.


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