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

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arxiv 1110.1847 v1 pith:AM7UOH44 submitted 2011-10-09 astro-ph.SR

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keywords possibleprogenitorsstarssymbioticaccretesaimsbinariesbinary
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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.

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  1. Symbiotic stars in the era of modern ground- and space-based surveys

    astro-ph.SR 2025-04 accept novelty 2.0 of 10

    A review of how large-scale photometric and spectroscopic surveys have transformed the discovery, classification, and variability studies of symbiotic stars.

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