Temperature and brightness distributions in the components of close binary system

Details Temperature and brightness distributions in the components of close binary system Temperature and brightness distributions in the components of close binary system

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991basi...19...59b&link_type=abstract

Astronomical Society of India, Bulletin (ISSN 0304-9523), vol. 19, Mar.-June 1991, p. 59-64.

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Brightness Distribution, Stellar Luminosity, Stellar Rotation, Stellar Temperature, Roche Limit, Stellar Gravitation, Stellar Models, Temperature Distribution

Scientific paper

A theoretical model of close binary system for the gravity-darkening due to tidally and nonuniformly rotating Roche components has been formulated using the fourth order of r/R where r is the radial distance and R is the distance between the centers of the binary stars. This model provides expressions to calculate the temperature and brightness distributions along the surface of the components.

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