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Nature. 2011 Dec 14;480(7377):348-50. doi: 10.1038/nature10646.

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

Author information

  • 1Department of Astronomy, University of California, Berkeley, California 94720-3411, USA. weidong@berkeley.edu

Abstract

Type Ia supernovae are thought to result from a thermonuclear explosion of an accreting white dwarf in a binary system, 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: double-degenerate (involving two white dwarfs in a close binary system) and single-degenerate models. 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. 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, allowing us to rule out luminous red giants and almost all helium stars as the mass-donating companion to the exploding white dwarf.

PMID:
22170681
[PubMed]
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