Diagnostics of circumstellar gas in Algol-type close binary systems

Details Diagnostics of circumstellar gas in Algol-type close binary systems Diagnostics of circumstellar gas in Algol-type close binary systems

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8....3p&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, no. 4, July-Aug. 1992, p. 3-16. In Russian.

Mathematics

Logic

1

Accretion Disks, Binary Stars, Interstellar Gas, Stellar Envelopes, Stellar Systems, Anisotropy, Kinematics, Physical Properties, Stellar Spectrophotometry, Stellar Temperature, Stellar Winds

Scientific paper

The physical properties of circumstellar gas in Algol-type semidetached systems are analyzed, and observational data are reviewed. It is found that the basic kinematic and morphological properties of the circumstellar and circumbinary gaseous media can be interpreted in terms of a strong anisotropic stellar wind, in accordance with the conception of Tout and Hall (1991).

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