NGC 2599 is a large spiral galaxy in the constellation of Cancer. Its velocity with respect to the cosmic microwave background is 4,997±17 km/s, which corresponds to a Hubble distance of 240.4 ± 16.9 Mly (73.70 ± 5.17 Mpc). It was discovered by German-British astronomer William Herschel on 16 November 1784. NGC 2599 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms. NGC 2599 is a galaxy whose nucleus shines brightly in the ultraviolet and is listed in the Markarian catalogue as Mrk 389.
Supernova One supernova has been observed in NGC 2599: SN 1965P (type unknown, mag. 15.7) was discovered by Howard S. Gates on 6 March 1965.
See also List of NGC objects (2001–3000)
References
External links Media related to NGC 2599 at Wikimedia Commons NGC 2599 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


