Date and Time of the Query: 2019-08-25 T08:00:16 PDT
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Notes for object NGC 5322

9 note(s) found in NED.

1. 2002MNRAS.329..877C
Re:GB6 J1349+6011
128-redshift from Falco et al. (1999); classification (Liner or Sy2) in
Ho et al. (1997); spectrum in Ho et al. (1995).

2. 1997ApJ...481..710C
Re:NGC 5322
A completely obscuring dust lane, which is most probably a nearly
edge-on disk perpendicular to the broad radio-jet (Hummel, van der Hulst,
& Dickey 1984), cuts the nucleus in two and hides the very center of the
galaxy. In the color map, the disk reaches a central value of V - I =
1.62 and remains on average about 0.25 mag redder than the surroundings.
A red excess is detected in the region adjacent to the disk, south of the
galaxy. The isophotal fitting within ~2.5" is completely dominated by the
strong dust absorption, as is clearly shown from the very large scatter
in both the Fourier terms and the position angle. Inspection of the
residual maps shows that the sharp decrease in ellipticity toward the
center is also an artifact of the fits. Outside 2.5", the fits reproduce
the morphology of the galaxy quite well. The ellipticity drops
significantly, together with C_4_, which drops from 0.02 to -0.005, which
indicates a transition from disky to boxy isophotes. This provides strong
evidence for an embedded stellar disk from ~1.5" out to ~8".

3. 1994CAG1..B...0000S
Re:NGC 5322
May 15/16, 1926
90 min
The classification of E4 for NGC 5322 is based on the early Mount
Wilson 60-inch plate shown here. An extended envelope exists, although
it is less pronounced than that of NGC 2685. NGC 5322 is near the
border of the E and E/S0 morphological boxes. It is noted in the RC1
that the classification is possibly S0^-^, based on the same 60-inch
plate used here.

4. 1994A&AS..105..481M
Re:NGC 5322
NGC 5322: A perfect model of boE with e_4_ < 0 throughout (except in
the innermost contours, l < 6 arcsec), while the axis-ratio regularly

5. 1994A&AS..105..341G
Re:NGC 5322
This boxy galaxy contains a stellar disk along its major axis in the
inner ~9" (cf. Paper I). Kim (1989) did already search for dust and
ionized gas in this galaxy, but reported no detection. However, our
H{alpha}+[NII] image reveals extended emission which is elongated along
the major axis and may thus be physically associated with this disk. Our
B-I image does not reveal obvious associated dust absorption. Detected by
IRAS at 60 and 100 microns. Radio source. X-ray emission.

6. 1994A&AS..104..179G
Re:NGC 5322
Stellar disk along major axis causes the positive C4 parameter (as well
as higher ellipticity) in the inner ~ 9". Boxy isophotes in the outer
regions (C4 ~ -0.01). Detected by IRAS at 60 & 100 microns. Radio source.
X-ray emission.

7. 1976RC2...C...0000d
Re:NGC 5322
Photometry (5 Color):
A.J., 73, 313, 1968.

8. 1973UGC...C...0000N
Re:UGC 08745
E3-4 (de Vaucouleurs)

9. 1964RC1...C...0000d
Re:NGC 5322
Bright diffuse nucleus. Smooth nebulosity. Possibly S0-?
Heidelberg Veroff. Vol. 9, 1926, Lund 9 and HA 88,2 dimensions are for the
bright part only.
Ap. J. 85, 325, 1937.

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