Date and Time of the Query: 2018-12-12 T21:00:15 PST
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Notes for object NGC 2196

9 note(s) found in NED.

1. 2005MNRAS.362.1319L
Re:NGC 2196
NGC 2196. This is a non-barred galaxy, but has an elliptical inner structure,
which is not completely aligned with the underlying disc. The inner elliptical
structure appears also as a strong m= 2 peak in the amplitude profile in the
Fourier analysis.

2. 2002ApJS..143...73E
Re:NGC 2196
NGC 2196.---S0/a: Bright nuclear point source embedded in bright
elliptical bulge. A very low surface brightness disk surrounds bulge.
The disk is smooth, with only a hint of some patchiness in the NW.

3. 2002AJ....123..159C
Re:NGC 2196
Spiral red (dust) feature southeast of center (down to reddened center)

4. 2001A&A...368...16M
Re:NGC 2196
5. NGC 2196 is a nearly face-on Sa/Sab galaxy. Carollo & Stiavelli (1998)
found on HST images the continuation of the R^1/4^ density profile of the
bulge to less than 1" radius. We obtained a slope of {beta} = 0.31 for the
whole bulge. The residua of our disk-bulge fit look good. The star near the
centre was extracted before the fit.

5. 1998AJ....116...68C
Re:NGC 2196
The surface brightness profile is reproduced either by an R^1/4^ law
plus exponential profile with parameters as in Table 2, or by a
single R^1/4^ law of ~30". Visual inspection of the image favors the
first interpretation, since spiral arms are present within 30".

6. 1994CAG1..B...0000S
Re:NGC 2196
Jan 30/31, 1979
103aO + GG385
45 min
The spiral arms in NGC 2196 are tightly wound about the large,
generally smooth central region (burned out in the print here) which,
nevertheless, has a series of very regular spiral arcs (formed by
dust) traceable to the center of the image. Present-day star formation
is evident in the two main outer arms.
The spiral arms here have features common to the two main types
of spiral patterns, the grand design and the multiple-armed-spiral
(MAS) types often described in the Sa section. The outer arms of NGC
2196 are of the grand design pattern. The many inside arm fragments
have a mini-MAS pattern, but one which is much less pronounced than in
the prototype MAS galaxies NGC 2775 (Sa; panels 78, 87, S12), NGC 4380
(Sab; panel 117), NGC 2268 (Sbc; panel 188), NGC 3953 (SBbc; panel
204), NGC 4689 (Sc; panel 277), NGC 4647 (Sc; panels 51, 278, 514),
and NGC 7793 (Sd; panels 321, S6), and the prototypes of the pattern
in NGC 2841 (Sb; panels 142, S4, S12), and NGC 488 (Sab; panels 115,
116, S3, S12).

7. 1985SGC...C...0000C
Re:NGC 2196
Plate 5481
Overexposed center, incomplete(?) (r): 1.0 x 0.65.
Knotty arms form (R'): 1.6 x 1.4.

8. 1974UGCA..C...0000N
Re:UGCA 121
UGCA 121:
= NGC 2196
(R')SA(s)a (RC1)

9. 1964RC1...C...0000d
Re:NGC 2196
Bright diffuse nucleus
in smooth bulge with faint smooth arcs forming
hexagonal pseudo (R): 1.5 arcmin x 1.4 arcmin,
slightly asymmetric

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