Detection of a red supergiant progenitor star of a type II - Plateau supernova

被引:167
作者
Smartt, SJ
Maund, JR
Hendry, MA
Tout, CA
Gilmore, GF
Mattila, S
Benn, CR
机构
[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[2] AlbaNova Univ Ctr, Stockholm Observ, SE-10691 Stockholm, Sweden
[3] Isaac Newton Grp Telescopes, E-38700 Santa Cruz De La Palma, Spain
关键词
D O I
10.1126/science.1092967
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
We present the discovery of a red supergiant star that exploded as supernova 2003gd in the nearby spiral galaxy M74. The Hubble Space Telescope (HST) and the Gemini Telescope imaged this galaxy 6 to 9 months before the supernova explosion, and subsequent HST images confirm the positional coincidence of the supernova with a single resolved star that is a red supergiant of 8(-2)(+4) solar masses. This confirms both stellar evolution models and supernova theories predicting that cool red supergiants are the immediate progenitor stars of type II-plateau supernovae.
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收藏
页码:499 / 503
页数:5
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