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Impact of Type Ia Supernova Ejecta on Binary Companions in the Single-degenerate Scenario

ASTROPHYSICAL JOURNAL, no. 2 (2012)

Cited: 78|Views24

Abstract

Type Ia supernovae are thought to be caused by thermonuclear explosions of a carbon-oxygen white dwarf in close binary systems. In the single-degenerate scenario (SDS), the companion star is non-degenerate and can be significantly affected by the explosion. We explore this interaction by means of multi-dimensional adaptive mesh refinement...More

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