SN 2007bi

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SN 2007bi
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Light curves for three photometric bands, plotted from data obtained from the Open Supernova Catalog[1]
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Right ascensionTemplate:RA
Declination+08° 55′ 44.3″
EpochJ2000.0
Galactic coordinates324.1496 +70.6427
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HostAnon J131920+0855[2]
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SN 2007bi was an extremely energetic supernova discovered early in 2007 by the international Nearby Supernova Factory based at the U.S. Department of Energy's Lawrence Berkeley National Laboratory. The precursor star is estimated to have had 200 solar masses at the time of its formation and around 100 solar masses in its core when it went supernova. The explosion ejected more than 22 solar masses of silicon and other heavy elements into space during this supernova including more than 6 solar masses of radioactive nickel which caused the expanding gases to glow very brightly for many months.[3]

The supernova has been described as an unambiguous fit for the pair-instability supernova model.[4]

References

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  1. ^ Page Module:Citation/CS1/styles.css has no content.Guillochon, James; Parrent, Jerod; Kelley, Luke Zoltan; Margutti, Raffaella (January 2017). "An Open Catalog for Supernova Data". The Astrophysical Journal. 835 (1): 64. arXiv:1605.01054. Bibcode:2017ApJ...835...64G. doi:10.3847/1538-4357/835/1/64.
  2. ^ Page Module:Citation/CS1/styles.css has no content."2007bi". SIMBAD. Centre de données astronomiques de Strasbourg. {{cite web}}: Invalid |mode=Script error: No such module "Citation mode". (help)
  3. ^ Page Module:Citation/CS1/styles.css has no content.David Shiga (2 December 2009). "Death of rare giant star sheds light on cosmic past". New Scientist.
  4. ^ Page Module:Citation/CS1/styles.css has no content.Gal-Yam, A.; Mazzali, P.; Ofek, E. O.; et al. (2009), "Supernova 2007bi as a pair-instability explosion", Nature, 462 (7273): 624–627, arXiv:1001.1156, Bibcode:2009Natur.462..624G, doi:10.1038/nature08579, PMID 19956255, S2CID 4336232

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