Light-curve Synthesis for Close Binaries Overfilling Their Inner Roche Lobes

Details Light-curve Synthesis for Close Binaries Overfilling Their Inner Roche Lobes Light-curve Synthesis for Close Binaries Overfilling Their Inner Roche Lobes

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002arep...46..740m&link_type=abstract

Astronomy Reports, Vol. 46, Issue 9, pp. 740-746

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a procedure for calculating theoretical monochromatic light curves of close binary systems overfilling their inner Roche lobes. The close binaries are considered in a Roche model with a cold spot on one of the components. The system radiation is calculated in both a blackbody approximation and using model stellar atmospheres, taking into account tidal deformations of the components, limb darkening, gravitational darkening, and the effect of mutual heating of the components.

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