Date and Time of the Query: 2019-06-16 T00:47:24 PDT
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Notes for object NGC 6810

9 note(s) found in NED.

1. 2006ApJS..164...52S
Re:NGC 6810
The H{alpha} image of this galaxy (Fig. 17, right) shows strong emission,
extended for ~1' along the N-S direction, in a rectangular region. This emission
is composed of several individual knots. Diffuse emission, extending over a
region of 80" in diameter, is seen along the SE-NW direction, possibly related
to outflows. Another interesting structure that can be seen in this image is a
half-ring of small knots, to the east of the rectangular region described above.
This ring extends along the major axis of the galaxy, has a diameter of ~100" in
the N-S direction, and lies along the border of a dust lane. Observations by
Hameed & Devereux (1999) found similar structures.

2. 2002AJ....123..159C
Re:NGC 6810
V image is saturated; nucleus bluer than in V-H color map; ubiquitous
dust in central region

3. 1998AJ....116...68C
Re:NGC 6810
Central few pixels in the WFPC2 images are saturated (central surface
brightness exceeds 12.2 mag arcsec ^-2^).

4. 1996A&AS..117..417H
Re:ESO 142- G 035
17. ESO 142-35 / NGC 6810: highly inclined. In B, large-scale dust lane
parallel to the major axis, and overall patchy appearance. In the NIR, complex
central structure, with i) pointed innermost isophotes, giving evidence for a
bright disk here, ii) a crescent-like bright feature at ~5" on the far side
(barely visible in B), which turned up to be the unobscured half of the
innermost bulge region (HSM95b), iii) the emergence of two spiral arms, and
iv) a large bulge, whose outer regions distort the outermost disk isophotes
(this far-reaching bulge is markedly different from the one visible in B on the
ESO-LV image; see, e.g., Simien et al. 1993).

5. 1994CAG1..B...0000S
Re:NGC 6810
Aug 7/8, 1980
103aO + GG385
45 min
The dust lanes silhouetted against the near
side of the highly inclined disk of NGC 6810
define the spiral structure. The arm pattern is
less open, and the star-formation rate is smaller
than in Sc types. The central bulge is smaller and
less smooth than in Sa types. The type is Sb by

6. 1985SGC...C...0000C
Re:NGC 6810
Plate 906
Strong dark lane. Similar to NGC 4594 with more dust.

7. 1982ESOU..C...0000L
Re:ESO 193921-5846.5
=ESO 142- G 35
absorption lane
in cluster

8. 1976RC2...C...0000d
Re:NGC 6810
Pair with large very faint galaxy 12 arcmin south-preceding.
Radio Observations:
Australian J. Phys., 21, 193, 1968.

9. 1964RC1...C...0000d
Re:NGC 6810
Very bright nucleus. Dark lane?
Pair with a large, very faint, anonymous galaxy 12 arcmin south-prceding.

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