Date and Time of the Query: 2019-04-22 T08:37:37 PDT
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Notes for object NGC 7463

7 note(s) found in NED.

1. 2005MNRAS.364.1253V
Re:NGC 7463
NGC 7463. This galaxy is part of a triple system with NGC 7464 (to the S of NGC
7463) and NGC 7465 (not shown in Fig. 1). At 850 {mu}m we clearly detect
emission from both NGC 7463 and 7464, which seem to be joined by a bridge of
submm emission. The flux listed in Table 1 is for NGC 7463 alone, measured in an
aperture corresponding to its main optical extent. Unfortunately, a very noisy
bolometer to the SE prevents us measuring the flux from the eastern half of NGC
7464, but excluding this region we measure a flux for the pair of 0.051+/-0.012
Jy, though obviously a lower limit.
An IRAS source is associated with NGC 7465, which is resolved from the other
members of the system at 60 {mu}m (HIRES; Aumann, Fowler & Melnyk 1990). Dust
properties of this system (using SCUBA data observed as part of SLUGS) are
studied in detail by Thomas et al. (2002).

2. 2002AJ....124..675C
Re:UGC 12316
F22954+1542 is a blend of UGC 12316 and UGC 12317.

3. 1985AnTok..202.237T
Re:KUG 2259+157A
In a pair with KUG 2259+157B. A spiral (KUG 2259+157A) and an almost
globular HII region (KUG 2259+157B) make a detached pair. In a triple
system with KUG 2259+156.

4. 1976RC2...C...0000d
Re:NGC 7463
= Holm 802a
Pair with NGC 7464 at 0.8 arcmin.
In a triple system with NGC 7464 and NGC 7465.

5. 1973UGC...C...0000N
Re:UGC 12316
See UGC 12315
UGC 12317 at 2.6, 115

6. 1964RC1...C...0000d
Re:NGC 7463
= Holm 802a

7. 1918PLicO..13....9C
Re:NGC 7463
2' x 0.3' in p.a; 95^deg^; moderately bright. No nucleus apparent. Very
irregular; the most prominent feature is a bright band cutting across the nebula
at an angle of about 50^deg^. Perhaps a {phi}-type spiral seen at a considerable

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