NGC 4541 is an intermediate spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 7,229±25 km/s, which corresponds to a Hubble distance of 347.8 ± 24.4 Mly (106.63 ± 7.47 Mpc). However, eight non-redshift measurements give a closer mean distance of 312.09 ± 9.57 Mly (95.688 ± 2.933 Mpc). It was discovered by German-British astronomer William Herschel on 1 January 1786. NGC 4541 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. NGC 4541 is also a radio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure.
Supernovae Two supernovae have been observed in NGC 4541:
SN 2007gq (type unknown, mag. 16.6) was discovered by Berto Monard on 4 August 2007. PTF11bpx (Type II, mag. 19.5) was discovered by the Palomar Transient Factory on 4 April 2011.
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4541 at Wikimedia Commons NGC 4541 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


