Methods for the synthesis of theoretical light curves of close binary systems

Details Methods for the synthesis of theoretical light curves of close binary systems Methods for the synthesis of theoretical light curves of close binary systems

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65.1164a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Nov.-Dec. 1988, p. 1164-1177. In Russian.

Statistics

Computation

19

Binary Stars, Computational Astrophysics, Light Curve, Roche Limit, Stellar Models, Stellar Atmospheres, Stellar Luminosity, Stellar Rotation, Stellar Temperature

Scientific paper

Algorithms are presented for the calculation of theoretical monochromatic light curves of close binaries within the framework of the Roche model and the geometrically thick disk model. Assumed to be present in the system is an extended semi-transparent atmosphere expanding with a constant velocity. Allowance is made for rotational and tidal distortion of the components, limb darkening, gravitational darkening, and the reflection effect.

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