NGC 664 is a spiral galaxy in the constellation of Pisces. Its velocity with respect to the cosmic microwave background is 5137 ± 21 km/s, which corresponds to a Hubble distance of 247.1 ± 17.3 Mly (75.77 ± 5.31 Mpc). In addition, six non redshift measurements give a closer distance of 218.91 ± 3.66 Mly (67.117 ± 1.123 Mpc). It was discovered by British astronomer John Herschel on 24 September 1830.
Supernovae Three supernovae have been observed in NGC 664:
SN 1996bw (Type II, mag. 17.5) was discovered by the BAO Supernova Survey on 30 November 1996. SN 1997W (Type II, mag. 18) was discovered by the Harvard–Smithsonian Center for Astrophysics on 1 February 1997. SN 1999eb (Type IIn, mag. 16.2) was discovered by the Lick Observatory Supernova Search (LOSS) on 2 October 1999.
NGC 664 Group NGC 664 is the namesake of the four member NGC 664 group. The other three galaxies are: IC 150, UGC 1204, and UGC 1240.
See also List of NGC objects (1–1000)
References
External links Media related to NGC 664 at Wikimedia Commons NGC 664 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


