NGC 4790 is a barred spiral galaxy located in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 1,679 ± 24 km/s (1,043 ± 15 mi/s), which corresponds to a Hubble distance of 80.8 ± 5.8 Mly (24.76 ± 1.77 Mpc) away from the Solar System. In addition, six non-redshift measurements give a distance of 74.75 ± 4.07 Mly (22.917 ± 1.249 Mpc). NGC 4790 was discovered on 25 March 1786 by German-British astronomer William Herschel. NGC 4790 is a member of the NGC 4699 Group (also known as LGG 307) of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.
Astronomical transients One astronomical transient event has been observed in NGC 4790: the supernova SN 2012au (Type Ib, mag. 13.8), which was discovered by the Catalina Sky Survey on 14 March 2012. This supernova later produced evidence of a pulsar wind nebula which appears to be expanding outward at approximately 2,300 km/s (1,400 mi/s).
Gallery
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4790 at Wikimedia Commons NGC 4790 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images SIMBAD entry NASA Extragalactic Database entry Messier45 entry Archived 2018-09-23 at the Wayback Machine VizieR




