Statistics – Computation
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992azh....69...58k&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 69, no. 1, Jan.-Feb. 1992, p. 58-70. In Russian.
Statistics
Computation
3
Accretion Disks, Binary Stars, Computational Astrophysics, Light Curve, Relativistic Effects, Astronomical Models, Roche Limit, Stellar Structure
Scientific paper
A method for synthesizing the light curve of a close binary system consisting of a normal star and a compact object is presented. The compact object is surrounded by an asymmetric disk of complex form: the disk is geometrically thin around the relativistic object and geometrically thick at the edge. The disk's asymmetry is due to its thickening in the region where the gaseous stream from the normal star filling its Roche lobe collides with the matter of the axisymmetric part of the disk.
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