NGC 3891 is a large spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background is 6,581±20 km/s, which corresponds to a Hubble distance of 316.6 ± 22.2 Mly (97.06 ± 6.80 Mpc). However, 10 non-redshift measurements give a slightly farther mean distance of 330.46 ± 14.72 Mly (101.320 ± 4.514 Mpc). It was discovered by German-British astronomer William Herschel on 3 February 1788. NGC 3891 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms. It is also a radio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure. NGC 3891 is a member of the Coma cluster.
Supernovae Two supernovae have been observed in NGC 3891:
SN 2006or (Type Ia, mag. 16.3) was discovered by Tim Puckett and A. Kroes on 18 November 2006. SN 2018bdv (Type II-P, mag. 18.53) was discovered by Gaia Photometric Science Alerts on 29 April 2018.
See also List of NGC objects (3001–4000)
References
External links Media related to NGC 3891 at Wikimedia Commons NGC 3891 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


