Companion Stars of Type Ia Supernovae

Abstract

The WD+MS channel of the single-degenerate scenario is currently favourable for progenitors of type Ia supernovae (SNe Ia). Incorporating the results of detailed binary evolution calculations for this channel into the latest version of a binary population synthesis code, I obtained the distributions of many properties of the companion stars at the moment of SN explosion. The properties can be verified by future observations.

arXiv comment7 figures, accepted for publication in ApJL

References in corpus (19)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• The Origin of Subdwarf B Star (I): the Formation Channels
• The origin of sdB stars (II)
• Two populations of progenitors for type Ia SNe?
• The single degenerate channel for the progenitors of type Ia supernovae
• A Wide Symbiotic Channel to Type Ia Supernovae
• Type Ia Supernova Explosions in Binary Systems: The Impact on the Secondary Star and its Consequences
• On the formation and evolution of black-hole binaries
• The binary progenitor of Tycho Brahe's 1572 supernova
• Direct Detection of Galactic Halo Dark Matter
• Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants?
• A Deep Chandra Observation of Kepler's Supernova Remnant: A Type Ia Event with Circumstellar Interaction
• A single-degenerate model for the progenitor of the Type Ia supernova 2002ic
• Type Ia Supernovae and High Velocity White Dwarfs
• Identification of the companion stars of Type Ia supernovae
• A Critical Examination of Halo White Dwarf Candidates
• On the Evolution and Appearance of a Surviving Companion after a Type Ia Supernova Explosion
• An ultra-cool white dwarf serendipitously found with COMBO-17

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• Blue Large-Amplitude Pulsators: the Possible Surviving Companions of Type Ia Supernovae
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• On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae
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• Hot subdwarfs from the surviving companions of the white dwarf + main-sequence channel of Type Ia supernovae