NGC 4219 is a spiral galaxy in the constellation of Centaurus. Its velocity with respect to the cosmic microwave background is 2,277±20 km/s, which corresponds to a Hubble distance of 109.6 ± 7.7 Mly (33.59 ± 2.37 Mpc). However, 16 non-redshift measurements give a closer mean distance of 72.00 ± 2.21 Mly (22.075 ± 0.679 Mpc). It was discovered by British astronomer John Herschel on 3 June 1834. NGC 4219 is a Seyfert I 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.
Supernovae Two supernovae have been observed in NGC 4219:
SN 2011am (Type Ib, mag. 17.4) was discovered by Australian amateur astronomer Stuart Parker on 27 February 2011. SN 2011hp (Type Ic, mag. 15.7) was discovered by South African amateur astronomer Berto Monard on 3 November 2011.
Image gallery
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4219 at Wikimedia Commons NGC 4219 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images



