NGC 278

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search
NGC 278
NGC 278 by HST
Observation data (J2000 epoch)
Constellation Cassiopeia
Right ascension 00h 52m 04.3s[1]
Declination +47° 33′ 02″[1]
Redshift 0.00209[1]
Helio radial velocity 627 ± 1 km/s[1]
Distance 38.5 Mly
(11.8 Mpc)[2]
Apparent magnitude (V) 11.5[1]
Type SAB(rs)b[1]
Apparent size (V) 2′.1 × 2′.0 [1]
Other designations
UGC 528,[1] PGC 3051[1]
See also: Galaxy, List of galaxies

NGC 278 is a spiral galaxy (barred for some authors[3]) in the constellation Cassiopeia. It has a H II nucleus.[4]


NGC 278 is a small and compact high-surface brightness galaxy with high star formation rate taking place in an inner ring with a radius of 2 kiloparsecs, that may have been triggered by the merger with a smaller companion.[5]



  1. ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 278. Retrieved 2007-02-01.
  2. ^ "Distance Results for NGC 278". NASA/IPAC Extragalactic Database. Retrieved 2010-05-03.
  3. ^ Garrido, O.; Marcelin, M.; Amram, P.; Boissin, O. (February 2003). "GHASP: An Hα kinematic survey of spiral and irregular galaxies. II. Velocity fields and rotation curves of 15 galaxies". Astronomy & Astrophysics. 399. pp. 51–61. Bibcode:2003A&A...399...51G. doi:10.1051/0004-6361:20021784.
  4. ^ Ho, Luis C.; Filippenko, Alexei V.; Sargent, Wallace L. W. (October 1997). "A Search for 'Dwarf' Seyfert Nuclei. III. Spectroscopic Parameters and Properties of the Host Galaxies". Astrophysical Journal Supplement. 112. p. 315. arXiv:astro-ph/9704107. Bibcode:1997ApJS..112..315H. doi:10.1086/313041.
  5. ^ Knapen, J. H.; Whyte, L. F.; de Blok, W. J. G.; van der Hulst, J. M. (August 2004). "The nuclear ring in the unbarred galaxy NGC 278: Result of a minor merger?". Astronomy & Astrophysics. 423. pp. 481–493. arXiv:astro-ph/0405107. Bibcode:2004A&A...423..481K. doi:10.1051/0004-6361:20034336.
  6. ^ "Cassiopeia's unusual resident".

Coordinates: Sky map 00h 52m 04.3s, +47° 33′ 02″