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Symbiotic Stars as Possible Progenitors of SNe Ia: Binary Parameters and Overall Outlook

Published online by Cambridge University Press:  17 January 2013

J. Mikołajewska
J. Mikołajewska*
Affiliation:
Copernicus Astronomical Center, Warsaw, Poland
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Abstract

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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.

Keywords

binaries: symbiotic — stars: novaecataclysmic variablesfundamental parametersmass lossevolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Issue S281: Binary Paths to Type Ia Supernovae Explosions , July 2011 , pp. 162 - 165
Copyright
Copyright © International Astronomical Union 2013

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