NGC 4027

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NGC 4027
NGC 4027.jpg
ESO image of NGC 4027 (mirrored).
Observation data (J2000 epoch)
Constellation Corvus
Right ascension 11h 59m 30.2s [1]
Declination −19° 15 55 [1]
Redshift 1671 ± 6 km/s [1]
Distance 83 Mly
(25.6 Mpc) [2]
Apparent magnitude  (V)11.7 [1]
Characteristics
Type SB(s)dm [1]
Apparent size  (V)3'.2 × 2'.4 [1]
Other designations
UGCA 260, PGC 37773, Arp 22,
VV 066, VIII Zw 158 [1]

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.

Contents

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

NGC 4027 with Hubble Arp 22 Hubble.jpg
NGC 4027 with Hubble

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

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<span class="mw-page-title-main">NGC 4221</span> Galaxy in constellation Draco

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References

  1. 1 2 3 4 5 6 7 "NASA/IPAC Extragalactic Database". Results for NGC 4027. Retrieved 2006-10-31.
  2. 1 2 "Distance Results for NGC 4027". NASA/IPAC Extragalactic Database. Retrieved 2010-05-16.
  3. Transient Name Server entry for SN 1996W. Retrieved 30 March 2023.
  4. R. B. Tully (1988). Nearby Galaxies Catalog. Cambridge: Cambridge University Press. ISBN   978-0-521-35299-4.
  5. P. Fouque; E. Gourgoulhon; P. Chamaraux; G. Paturel (1992). "Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members". Astronomy and Astrophysics Supplement. 93: 211–233. Bibcode:1992A&AS...93..211F.
  6. A. Garcia (1993). "General study of group membership. II - Determination of nearby groups". Astronomy and Astrophysics Supplement. 100: 47–90. Bibcode:1993A&AS..100...47G.
  7. G. Giuricin; C. Marinoni; L. Ceriani; A. Pisani (2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". Astrophysical Journal. 543 (1): 178–194. arXiv: astro-ph/0001140 . Bibcode:2000ApJ...543..178G. doi:10.1086/317070. S2CID   9618325.