Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe

Article

关键词: WHITE-DWARF MODELS;    IA SUPERNOVAE;    X-RAY;    RECURRENT NOVAE;    EVOLUTION;    MASS;    BINARIES;    CHANNEL;    DISTANCE;    SYSTEM;   

DOI  :  10.1038/nature10646

来源: SCIE

【 摘 要 】

Type Ia supernovae are thought to result from a thermonuclear explosion of an accreting white dwarf in a binary system(1,2), but little is known of the precise nature of the companion star and the physical properties of the progenitor system. There are two classes of models(1,3): double-degenerate (involving two white dwarfs in a close binary system(2,4)) and single-degenerate models(5,6). In the latter, the primary white dwarf accretes material from a secondary companion until conditions are such that carbon ignites, at a mass of 1.38 times the mass of the Sun. The type Ia supernova SN 2011fe was recently detected in a nearby galaxy(7). Here we report an analysis of archival images of the location of SN 2011fe. The luminosity of the progenitor system (especially the companion star) is 10-100 times fainter than previous limits on other type Ia supernova progenitor systems(8-10), allowing us to rule out luminous red giants and almost all helium stars as the mass-donating companion to the exploding white dwarf.

【 授权许可】

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