Synthesis of Lightcurves of Close Binary Systems Containing a Relativistic Object - Asymmetric Geometrically Thick Disk around the Relativistic Objectстатья
Дата последнего поиска статьи во внешних источниках: 28 мая 2015 г.
Аннотация:The method is given for synthesizing the light curve of a close binary system consisting of a normal star and a compact object surrounded by an asymmetric disk of complicated shape: geometrically thin near the relativistic object and geometrically thick at the edge of the disk. The asymmetry of the disk is caused by its thickening in the region of collision between matter flowing from the normal star, which fills its Roche lobe, and matter in the axisymmetric part of the disk.