Computer Science – Numerical Analysis
Scientific paper
Dec 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68.1211k&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Nov.-Dec. 1991, p. 1211-1226. In Russian.
Computer Science
Numerical Analysis
6
Accretion Disks, Binary Stars, Light Curve, Mathematical Models, Numerical Analysis
Scientific paper
A method for light-curve synthesis of close binary systems which consist of a normal star and a compact object is given. The compact object is surrounded by an axisymmetric disk of complex form: the disk is geometrically thin around the relativistic object and geometrically thick at the edge. The possible presence of a bright spot on the disk's lateral surface is taken into account. This spot may appear as a result of a collision between the gaseous stream from a normal star that fills its Roche lobe and the disk's matter.
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