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

被引：164

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

来源：

SCIENCE | 2004年 / 303卷 / 5657期

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.

引用

页码：499 / 503

页数：5

共 42 条

[1] SN 1993J - THE OPTICAL-PROPERTIES OF ITS PROGENITOR [J].