Arp 273 Explained

Arp 273
Type:SA(s)b pec + SB(s)a pec
Epoch:J2000
Dist Ly:300 million ly
Appmag V:13.7
Constellation Name:Andromeda
Names:, VV 323a

Arp 273 is a pair of interacting galaxies, 300 million light years away in the constellation Andromeda. It was first described in the Atlas of Peculiar Galaxies, compiled by Halton Arp in 1966. The larger of the spiral galaxies, known as UGC 1810, is about five times more massive than the smaller galaxy. It has a disc that is tidally distorted into a rose-like shape by the gravitational pull of the companion galaxy below it, known as UGC 1813. The smaller galaxy shows distinct signs of active star formation at its nucleus, and "it is thought that the smaller galaxy has actually passed through the larger one."

One supernova has been observed in UGC 1810: SN 1962R (type unknown, mag. 15.9).[1]

External links

Notes and References

  1. https://www.wis-tns.org/object/1962R Transient Name Server entry for SN 1962R.