Comparison between two-and three-dimensional modeling of the structure of an accretion disk in a binary system |
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Authors: | M V Abakumov S I Mukhin Yu P Popov V M Chechetkin |
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Institution: | (1) Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Miusskaya pl. 4, Moscow, 125047, Russia |
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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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