Galaxy in the constellation Pisces
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).[1] In addition, six non redshift measurements give a distance of 218.91 ± 3.66 Mly (67.117 ± 1.123 Mpc).[2] It was discovered by British astronomer John Herschel on 24 September 1830.[3]
Supernovae
Three supernovae have been observed in NGC 664:
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.[10]
See also
References
- ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for object NGC 664. Retrieved 22 August 2024.
- ^ "Distance Results for NGC 664". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 22 August 2024.
- ^ Seligman, Courtney. "NGC 664". Celestial Atlas. Retrieved 22 August 2024.
- ^ Li, W.; Qiao, Q.; Qiu, Y.; Hu, J.; Wei, J.; Xiu, D. (1996). "Supernova 1996bw in NGC 664". International Astronomical Union Circular (6512): 1. Bibcode:1996IAUC.6512....1L.
- ^ "SN 1996bw". Transient Name Server. IAU. Retrieved 22 August 2024.
- ^ Berlind, P.; Garnavich, P.; Hergenrother, C. (1997). "Supernovae 1997W and 1996bw in NGC 664". International Astronomical Union Circular (6551): 1. Bibcode:1997IAUC.6551....1B.
- ^ "SN 1997W". Transient Name Server. IAU. Retrieved 22 August 2024.
- ^ Modjaz, M.; Li, W. D.; Garnavich, P.; Jha, S.; Challis, P.; Kirshner, R.; Berlind, P. (1999). "Supernova 1999eb in NGC 664". International Astronomical Union Circular (7268): 1. Bibcode:1999IAUC.7268....1M.
- ^ "SN 1999eb". Transient Name Server. IAU. Retrieved 22 August 2024.
- ^ Zabludoff, Ann I.; Mulchaey, John S. (1998). "The Properties of Poor Groups of Galaxies. I. Spectroscopic Survey and Results". The Astrophysical Journal. 496 (1): 39–72. arXiv:astro-ph/9708132. Bibcode:1998ApJ...496...39Z. doi:10.1086/305355.
External links