Physics
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.196..241d&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 196, no. 2, p. 241-265, 267-282.
Physics
36
Accretion Disks, Astronomical Photometry, Eclipsing Binary Stars, Light Curve, Starspots, Stellar Models, Stellar Orbits, Optical Thickness, Radiant Flux Density, Stellar Activity, Stellar Physics, Stellar Radiation
Scientific paper
The actual problematics in the determination of orbital and physical parameters of active CB on the basis of the interpretation of photometric observations are presented. The basis of the model developed for the synthesis of asymmetric, deformed, light curves of active CB with spots on their components is described. The system components are considered in the framework of the nonsynchronous Roche model and the accretion disk of a constant thickness lies in the orbital plane about the star capturing the matter of the neighboring component.
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