Symbiotic Novae
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The symbiotic novae are thermonuclear novae in symbiotic binary systems -- interacting binaries with evolved red giant donors, and the longest orbital periods. This paper aims at presenting physical characteristics of these objects and discussing their place among the whole family of symbiotic stars.
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Cited by 3 Pith papers
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Millimeter-wave Detections of Symbiotic Stars in SPT and ACT Data
Millimeter detections of 31 symbiotic stars yield light curves and evidence of lagged variability in one source, supporting tests of binary models via free-free and dust emission.
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Millimeter-wave Detections of Symbiotic Stars in SPT and ACT Data
31 symbiotic stars detected above 3σ at 95-220 GHz in SPT/ACT data, with light curves, SEDs, and upper limits provided for candidates.
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New Online Database of Symbiotic Variables: Catalog and Statistical Overview of Symbiotic Binaries
NODSV is a new public catalog of ~1400 symbiotic binaries with classifications into confirmed, candidate, and misidentified categories plus a statistical overview of their properties.
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