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Symbiotic stars as possible progenitors of SNe Ia: binary parameters and overall outlook
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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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Symbiotic stars in the era of modern ground- and space-based surveys
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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