Jump to content

NGC 4881

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by InternetArchiveBot (talk | contribs) at 03:37, 12 April 2020 (Rescuing 1 sources and tagging 0 as dead.) #IABot (v2.0). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

NGC 4881
Elliptical Galaxy NGC 4881 (center) and the Spiral galaxy PGC 44691 (right).
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 59m 57.6s[1]
Declination+28° 14′ 51″[1]
Redshift0.022482±0.000019
Heliocentric radial velocity6740±6 km/s[1]
Galactocentric velocity6755±6 km/s[1]
Distance352 Mly[citation needed]
Apparent magnitude (V)14.6[1]
Characteristics
TypeE[1]
Apparent size (V)1′.0 × 1′.0[1]
Other designations
UGC 8106,[1] PGC 44686[1]

NGC 4881 is an elliptical galaxy about 102 megaparsecs away in the Coma cluster of galaxies.[2] NGC 4881 was discovered by Heinrich Louis d'Arrest in 1865.

In 1994, the Hubble Space Telescope examined the Coma cluster and NGC 4881.[3]

Other resources

See also

References

  1. ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 4881. Retrieved 2017-11-02.
  2. ^ Thomsen, Bjarne; Baum, William A.; Hammergren, Mark; Worthey, Guy (1997). "The Distance to the Coma Cluster from Surface Brightness Fluctuations". The Astrophysical Journal. 483 (1): L37–L40. arXiv:astro-ph/9704121. Bibcode:1997ApJ...483L..37T. doi:10.1086/310735. ISSN 0004-637X.
  3. ^ "Ngc 4881".