A review of the ultraviolet results about symbiotic stars

Details A review of the ultraviolet results about symbiotic stars A review of the ultraviolet results about symbiotic stars

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..203f&link_type=abstract

In ESA 3rd European IUE Conf. p 203-208 (SEE N83-11889 02-88)

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Stellar Models, Stellar Spectra, Ultraviolet Spectra, Variability, Accretion Disks, Hot Stars, Stellar Envelopes, Stellar Luminosity, Stellar Mass Accretion, Stellar Winds

Scientific paper

Ultraviolet properties of the symbiotic stars, and results on AG Dra and other objects, are discussed. Different single and binary model are examined: hot star surrounded by a cool envelope; cool star with a hot envelope; and binary systems. Accretion disks seem to play a role in some cases. Stellar winds from both components, but especially from the cool one, must be taken into account. There is evidence of excess heating of the outer layers of the cool component.

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