Light Curve Solution for Early-type Binary Systems with Radiative Interaction

Details Light Curve Solution for Early-type Binary Systems with Radiative Interaction Light Curve Solution for Early-type Binary Systems with Radiative Interaction

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006javso..35..174d&link_type=abstract

The Journal of the American Association of Variable Star Observers, Vol. 35, No. 1, p. 174-176

Computer Science

Scientific paper

An eclipse light curve analysis code based on the logistics of the Wilson-Devinney approach has been developed to account for the effects of radiation pressure due to the mutual irradiation of the components of close binary systems. The radiative forces exerted by luminous, hot stars may cause geometric deformations of stellar surfaces and influence the binary configuration and evolution.

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