NGC 4027 explained

NGC 4027
Epoch:J2000
Ra:[1]
Constellation Name:Corvus
Z:1671 ± 6 km/s
Dist Ly:83 Mly
[2]
Type:SB(s)dm
Appmag V:11.7
Size V:3'.2 × 2'.4
Names:UGCA 260, PGC 37773, Arp 22,
VV 066, VIII Zw 158

NGC 4027 (also known as Arp 22) is a barred spiral galaxy approximately 83 million light-years away[2] in the constellation Corvus. It is also a peculiar galaxy because one of its spiral arms goes out more than the other. This is probably due to a galactic collision in NGC 4027's past.

One supernova has been observed in NGC 4027: SN 1996W (type II, mag. 16).[3]

Galaxy group information

NGC 4027 is part of the NGC 4038 Group, a group of galaxies that also contains the Antennae Galaxies (NGC 4038/NGC 4039).[4] [5] [6] [7]

See also

External links

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 4027 . 2006-10-31.
  2. Web site: Distance Results for NGC 4027 . NASA/IPAC Extragalactic Database . 2010-05-16.
  3. https://www.wis-tns.org/object/1996W Transient Name Server entry for SN 1996W.
  4. Book: R. B. Tully . 1988 . Nearby Galaxies Catalog . . Cambridge . 978-0-521-35299-4.
  5. P. Fouque . E. Gourgoulhon . P. Chamaraux . G. Paturel . Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members . Astronomy and Astrophysics Supplement . 1992 . 93 . 211–233 . 1992A&AS...93..211F .
  6. A. Garcia . General study of group membership. II - Determination of nearby groups . Astronomy and Astrophysics Supplement . 1993 . 100 . 47–90 . 1993A&AS..100...47G.
  7. G. Giuricin . C. Marinoni . L. Ceriani . A. Pisani . Nearby Optical Galaxies: Selection of the Sample and Identification of Groups . Astrophysical Journal . 2000 . 543 . 1 . 178–194 . 2000ApJ...543..178G . 10.1086/317070. astro-ph/0001140 . 9618325 .