NGC 1156 explained

NGC 1156
Epoch:J2000
Type:IB(s)m[1]
Z:375 ± 1 km/s
Appmag V:12.3
Size V:3.3 × 2.5
Constellation Name:Aries
Names:UGC 2455, PGC 11329

NGC 1156 is a dwarf irregular galaxy in the Aries constellation of the type . It is considered a Magellanic-type irregular. The galaxy has a larger than average core, and contains zones of contra-rotating gas. The counter-rotation is thought to be the result of tidal interactions with another gas rich galaxy some time in the past.

It has a H II nucleus.[2]

The AGES survey has discovered a candidate dark galaxy close to NGC 1156, one of only a few so far found.

External links

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 1156 . 2006-11-27 .
  2. News: Ho . Luis C. . Filippenko . Alexei V. . Sargent . Wallace L. W. . A Search for "Dwarf" Seyfert Nuclei. III. Spectroscopic Parameters and Properties of the Host Galaxies . October 1997 . Astrophysical Journal Supplement . 112 . 2 . 315–390 . 10.1086/313041 . astro-ph/9704107 . 1997ApJS..112..315H .