NGC 4419 is a barred spiral galaxy in the constellation of Coma Berenices. It was discovered by German-British astronomer William Herschel on 8 April 1784. NGC 4419 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.
Distance NGC 4419 has a velocity with respect to the cosmic microwave background of 64±23 km/s, which is too small to be used to estimate its distance. Instead, 22 non-redshift measurements are used to give a mean distance of 52.49 ± 2.51 Mly (16.095 ± 0.771 Mpc).
Supernovae Two supernovae have been observed in NGC 4419:
SN 1984A (Type Ia, mag. 16) was discovered by Givi N. Kimeridze on 4 January 1984, and independently by Leonida Rosino on 7 January 1984. SN 2012cc (Type II, mag. 18.2) was discovered by the Lick Observatory Supernova Search (LOSS) on 29 April 2012.
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4419 at Wikimedia Commons NGC 4419 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


