NGC 2608
NGC 2608 (also known as Arp 12) is a barred spiral galaxy located 93 million light-years away in the constellation Cancer (the Crab). It is 62,000 light-years across, and about 60% of the width of the Milky Way. It is considered a grand design spiral galaxy and is classified as SB(s)b, meaning that the galaxy's arms wind moderately (neither tightly nor loosely) around the prominent central bar.
NGC 2608 | |
---|---|
Hubble Space Telescope image of NGC 2608 | |
Observation data (J2000 epoch) | |
Constellation | Cancer |
Right ascension | 08h 35m 17.3s [1] |
Declination | +28° 28′ 24″ [1] |
Redshift | 0.007122 (2135±8 km/s)[1] |
Distance | 93.0 Mly (28.5 Mpc) [2] |
Apparent magnitude (V) | 13.01 [1] |
Characteristics | |
Type | SB(s)b [1] |
Apparent size (V) | 2.3 × 1.4 arcmin [1] |
Other designations | |
Arp 012, PGC 024111 |
It was classified by Halton Arp under "galaxies with split arms" in his 1966 Atlas of Peculiar Galaxies who noted that the "nucleus may be double or superposed star."[3] NGC 2608 is now considered to be a pair of interacting galaxies.[4]
Supernovae
- SN 1920A was discovered by German astronomer Max Wolf (1863-1932). It peaked at magnitude 11.7 on 17 Dec 1920.[1] Its visual magnitude implies an overluminous bolometric magnitude; SN 1920A has since been classified as anomalous and is believed to be the result of "a completely different explosion mechanism."[5]
- SN 2001bg was discovered on 9 May 2001 (May 8.943 UT) by noted supernova hunter Tom Boles of Coddenham, Suffolk, England, with a 0.36-m Schmidt-Cassegrain telescope.[6] When first observed it was magnitude 14; it later peaked at around 13.7.[7] Its spectrum indicates that it is a typical Type Ia supernova.[1]
References
- "NASA/IPAC Extragalactic Database". Results for NGC 2608. Retrieved 7 Dec 2008.
- Seigar, Marc S. (Jul 2005). "The connection between shear and star formation in spiral galaxies". Monthly Notices of the Royal Astronomical Society: Letters. 361 (1): L20–L24. arXiv:astro-ph/0504529. Bibcode:2005MNRAS.361L..20S. doi:10.1111/j.1745-3933.2005.00056.x.
- Halton Arp (Nov 1966). "Atlas of Peculiar Galaxies". Astrophysical Journal Supplement. 14: 1. Bibcode:1966ApJS...14....1A. doi:10.1086/190147.
- "NGC 2608". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 Dec 2008.
- Schaefer, Bradley E.; Girard, Terrence M. (1999). "Weird Supernovae: Superluminous, Superfast and Superfaint Examples". Anni Mirabiles, A Symposium Celebrating the 90th Birthday of Dorrit Hoffleit Held 7–8 March 1997 at Yale University, New Haven, CT.: 69–70. Bibcode:1999anmi.conf...69S.
- "International Astronomical Union Circular". Supernova 2001bg in NGC 2608. Central Bureau for Astronomical Telegrams. 9 May 2001. Retrieved 8 Dec 2008.
- "2001 Annual Report". Central Bureau of Astronomical Telegrams. 2002. Retrieved 2011-07-05.
External links
Wikimedia Commons has media related to NGC 2608. |
- NGC 2608 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.