NGC 1201 is a lenticular galaxy in the constellation of Fornax. Its velocity with respect to the cosmic microwave background is 1,531±16 km/s, which corresponds to a Hubble distance of 73.6 ± 5.3 Mly (22.58 ± 1.61 Mpc). However, 10 non-redshift measurements give a closer mean distance of 63.37 ± 4.96 Mly (19.430 ± 1.520 Mpc). It was discovered by German-British astronomer William Herschel on 26 October 1785. NGC 1201 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
NGC 1255 group NGC 1201 is a member of the NGC 1255 group (also known as LGG 86), which contains at least 5 galaxies, including NGC 1255, NGC 1302, UGCA 61, and UGCA 64.
Supernova One supernova has been observed in NGC 1201:
SN 2003hv (Type Ia, mag. 12.5) was discovered by LOTOSS (Lick Observatory and Tenagra Observatory Supernova Searches) on 2 April 2003. It reached magnitude 12.3, making it the brightest supernova of 2003.
See also List of NGC objects (1001–2000)
References
External links Media related to NGC 1201 at Wikimedia Commons NGC 1201 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


