Synthesis of Lightcurves of Close Binary Systems Containing a Relativistic Object - Axisymmetric 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 axisymmetric disk of complicated shape: geometrically thin near the relativistic object and geometrically thick at the edge of the disk. Allowance is made for the possible presence of a hot spot on the lateral surface of the disk, originating from the collision between disk matter and matter flowing from the normal star, which fills its Roche lobe.