IC 167

IC 167
Observation data (J2000 epoch)
Constellation Aries
Right ascension 01h 51m 08.65s
Declination +21° 54 44.8
Redshift 0.00982 ± 0.00017
Apparent magnitude (V) 14.0
Characteristics
Type SBc
Apparent size (V) 3.09 × 1.862
Other designations
Arp 31, LEDA 6833, MCG+04-05-021, Z 0148.3+2140, APG 31, 2MASX1 J0151084+215447, UGC 1313, Z 482-25, LCSB L76, 2MASX J01510855+2154461, UZC J015108.6+215445

IC 167 is a barred spiral galaxy in the constellation of Aries. It was first reported by Bigourdan in 1891[1] and included in Dreyer's first Index Catalogue.[2]

Galaxy group information

IC 167 is a member of the NGC 697 group.[3] There is some evidence that IC 167 is interacting with nearby NGC 694 as they seem to share HI regions.[3] The tidal warping of IC 167 also is indicative of an interaction with another galaxy.[3] How long the interaction between these two galaxies has been occurring is the subject of current research.[4]

References

  1. Bigourdan, Guillaume (1891). "Nebuleuses nouvelles, decouvertes a l'Obseratoire de Paris" (PDF). Comptes Rendus Hebdomadaires de l'Académie des Sciences. 112: 647–650. Retrieved 29 December 2010.
  2. Dreyer, J.L.E. (1895). "Index Catalogue of Nebulae found in the years 1888 to 1894, with Notes and Corrections to the New General Catalogue". Mem. R. Astron. Soc. 51: 185–228. Bibcode:1895MmRAS..51..185D. Retrieved 29 December 2010.
  3. 1 2 3 van Moorsel, G.A. (1988). "A neutral hydrogen study of interacting galaxies in the NGC 697 group". Astronomy & Astrophysics. 202: 59–69. Bibcode:1988A&A...202...59V.
  4. Iyer, Mansie G.; Simpson, Caroline E.; Gottesman, Stephen T.; Malphrus, Benjamin K. (September 2004). "Neutral hydrogen in ARP 158". Astronomical Journal. 128: 985–996. arXiv:astro-ph/0405405Freely accessible. Bibcode:2004AJ....128..985I. doi:10.1086/422731.

External links

Coordinates: 01h 51m 08.65s, +21° 54′ 44.8″

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