Parameters of the eclipsing Wolf-Rayet binary system CQ CEP

Details Parameters of the eclipsing Wolf-Rayet binary system CQ CEP Parameters of the eclipsing Wolf-Rayet binary system CQ CEP

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65.1016a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Sept.-Oct. 1988, p. 1016-1027. In Russian.

Physics

7

Eclipsing Binary Stars, Light Curve, Stellar Physics, Stellar Spectrophotometry, Wolf-Rayet Stars, Mass Ratios, O Stars, Roche Limit, Stellar Mass

Scientific paper

The light curves of the system CQ Cep are interpreted using a Roche
model with an extended radially expanded atmosphere around the star WN7.
Information on the distance (3.5 kpc) and mass function of the WN7 star
is used to determine the basic parameters of the system.

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