M109 Group

M109 Group
Observation data (Epoch J2000)
Constellation(s)Ursa Major
Right ascension11h 55m [1][2]
Declination+51° 20′[1][2]
Brightest memberMessier 109[1][2]
Number of galaxies41–58[1][2][3]
Other designations
NGC 3992 Group, LGG 258,[1]
NOGG H 547,[2]
NOGG P1 588,[2] NOGG P2 597[2]

The M109 Group (also known as the NGC 3992 Group or Ursa Major cloud) is a group of galaxies about 55 million light-years away[4] in the constellation Ursa Major. The group is named after the brightest galaxy within the group, the spiral galaxy M109.

NGC 3982.
NGC 4157, seen by the 32 inch Schulman Foundation telescope on Mt. Lemmon, USA.
  1. ^ a b c d e 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.
  2. ^ a b c d e f g 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.
  3. ^ Cite error: The named reference nbg was invoked but never defined (see the help page).
  4. ^ The Ursa Major Groups