The AG Dra: A case of a stellar wind accretor

Details The AG Dra: A case of a stellar wind accretor The AG Dra: A case of a stellar wind accretor

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..109l&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 109-112 (SEE N86-20287 10-93)

Computer Science

3

Stellar Mass Accretion, Stellar Winds, Symbiotic Stars, Accretion Disks, Cataclysmic Variables, Stellar Spectra, Stellar Spectrophotometry

Scientific paper

Optical observations of the symbiotic star AG Dra indicate the presence of an accretion luminous disk in the system. The disk is fed by stellar wind from the cool component in the system. The binary revolution of the hot component within the nontransparent wind may account for the observed optical light curve of the system in the U, B and V photometric bands.

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