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Comparison between two-and three-dimensional modeling of the structure of an accretion disk in a binary system
Authors:M V Abakumov  S I Mukhin  Yu P Popov  V M Chechetkin
Institution:(1) Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Miusskaya pl. 4, Moscow, 125047, Russia
Abstract:We compare two-and three-dimensional modeling of gas-dynamical processes in the accretion disk of a binary system. The origin of spiral waves and the loss of the angular momentum related to them are considered. It is concluded that a steady state of the disk cannot exist without taking into account t he gas inflow from the donor star.
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