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Three-dimensional numerical simulation of gaseous flow structure in semidetached binaries
Authors:D V Bisikalo  A A Boyarchuk  V M Chechetkin  O A Kuznetsov  & D Molteni
Institution:Institute of Astronomy of Russian Academy of Sciences, 48 Pyatnitskaya str., Moscow 109017, Russia,;Keldysh Institute of Applied Mathematics, 4 Miusskaya sq., Moscow 125047, Russia,;Dipartimento di Scienze Fisiche ed Astronomiche, Universitàdi Palermo, 36 Via Archirafi, I-90123 Palermo, Italy
Abstract:
Keywords:accretion  accretion discs  hydrodynamics  methods: numerical  binaries: close  stars: mass-loss
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