Symbiotic stars as possible progenitors of SNe Ia: binary parameters and overall outlook

Details Symbiotic stars as possible progenitors of SNe Ia: binary parameters and overall outlook Symbiotic stars as possible progenitors of SNe Ia: binary parameters and overall outlook

2011-10-09

arxiv.org/abs/1110.1847v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages. Invited rewiev at "Binary Paths to Type Ia Supernovae", IAU Symposium No. 281, R. Di Stefano & M. Orio, eds., Cambrid

Scientific paper

Symbiotic stars are interacting binaries in which the first-formed white
dwarf accretes and burns material from a red giant companion. This paper aims
at presenting physical characteristics of these objects and discussing their
possible link with progenitors of type Ia supernovae.

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