SN 2002bj
 Light curves in four photometric bands for SN 2002bj, plotted from data published by Poznanski et al.[1] | |
| Event type | Supernova, variable star  |
|---|---|
| SN.IIn | |
| Constellation | Lepus |
| Right ascension | 05h 11m 46.41s[2] |
| Declination | −15° 08′ 10.8″[2] |
| Epoch | J2000 |
| Other designations | SN 2002bj, AAVSO 0507-15 |
SN 2002bj was the explosion of a star in the galaxy NGC 1821, located in the constellation Lepus.[3] The explosion was discovered by Jack Newton in scans of images produced by Tim Puckett. (It was independently discovered by the Lick/Tenagra Observatory as part of their combined supernova search program.) Initially it had an apparent magnitude of about 14.7[4] and was categorized as a Type IIn supernova.[5] However, in 2008 Dovi Poznanski discovered that the spectrum more closely resembled a Type Ia supernova. Further, the energy output was much lower than a typical supernova and the luminosity dropped at a dramatic pace.[6]
A team consisting of Poznanski, Joshua Bloom, Alex Filippenko and others concluded that it was a new category of exploding star. This system is believed to consist of a binary pair of white dwarf stars, with helium being transferred from one dwarf to the other. The accreted helium exploded in a thermonuclear reaction on the surface of the more massive white dwarf, resulting in the observed outburst.[6] In this sense, it was akin to a nova explosion, although the magnitude of the explosion was a thousand times greater.[3] In 2007 Lars Bildsten et al. had predicted this category of explosion would occur in AM Canum Venaticorum star binary systems.[7]
NGC 1821 is an irregular galaxy categorized as type IB(s)m. It is apparent magnitude 14.5 and has a redshift of 0.012029. This galaxy is located about 48 megaparsecs from the Earth.[8]
References
[edit]- ^ Poznanski, Dovi; Chornock, Ryan; Nugent, Peter E.; Bloom, Joshua S.; Filippenko, Alexei V.; Ganeshalingam, Mohan; Leonard, Douglas C.; Li, Weidong; Thomas, Rollin C. (January 2010). "An Unusually Fast-Evolving Supernova". Science. 327 (5961): 58. arXiv:0911.2699. Bibcode:2010Sci...327...58P. doi:10.1126/science.1181709. Retrieved 27 May 2025.
- ^ a b "SN 2002bj". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-01-25.
- ^ a b Sanders, Robert. "Rapid supernova could be new class of exploding star". UC Newsroom. University of California, Berkeley. Archived from the original on 2011-06-13. Retrieved 2009-11-06.
- ^ Bishop, David (Apr 26, 2002). "Supernova 2002bj in NGC 1821". Astronomy Section, Rochester Academy of Science. Retrieved 2009-11-06.
- ^ Matheson, T.; Berlind, P. (March 2002). "Supernova 2002bj in NGC 1821". IAU Circular. 7844 (5): 5. Bibcode:2002IAUC.7844....5M.
- ^ a b Siegel-Itzkovich, Judy (November 5, 2009). "US-Israeli team's speedily evolving supernova seems to be a new class of exploding star". The Jerusalem Post. Retrieved 2009-11-06.[permanent dead link]
- ^ Bildsten, Lars; Shen, Ken J.; Weinberg, Nevin N.; Nelemans, Gijs (June 2007). "Faint Thermonuclear Supernovae from AM Canum Venaticorum Binaries". The Astrophysical Journal. 662 (2): L95 – L98. arXiv:astro-ph/0703578. Bibcode:2007ApJ...662L..95B. doi:10.1086/519489. S2CID 119369896.
- ^ "NED results for object NGC 1821". NASA/IPAC Extragalactic Database. Retrieved 2009-11-06.
External links
[edit]- Light curves and spectra Archived 2017-12-02 at the Wayback Machine on the Open Supernova Catalog Archived 2016-03-03 at the Wayback Machine