NGC 4619 is a barred spiral galaxy in the constellation of Canes Venatici. Its velocity with respect to the cosmic microwave background is 7,176±18 km/s, which corresponds to a Hubble distance of 345.2 ± 24.2 Mly (105.84 ± 7.41 Mpc). However, 15 non-redshift measurements give a closer mean distance of 331.74 ± 12.34 Mly (101.713 ± 3.783 Mpc). It was discovered by German-British astronomer William Herschel on 1 May 1785. NGC 4619 is a Seyfert II galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.
Supernova One supernova has been observed in NGC 4619:
SN 2006ac (Type Ia, mag. 16.0) was discovered by the Lick Observatory Supernova Search (LOSS) on 9 February 2006.
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4619 at Wikimedia Commons NGC 4619 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


