|
Preprints of the Keldysh Institute of Applied Mathematics, 1998, 041
(Mi ipmp1355)
|
|
|
|
Comparison of 2d and 3d Models of Flow Structure in Semidetached Binaries
D. V. Bisikalo, A. A. Boyarchuk, O. A. Kuznetsov, D. Molteni, V. M. Chechetkin
Abstract:
We present the results of systematic comparison of 2D and 3D numerical models of mass transfer in semidetached binaries. It is shown that only for case of $\gamma$ 1 (near-isothermal case) the obtained 2D and 3D solutions are qualitatively similar. For higher value of $\gamma$ the 3D flow structure is drastically changed and for $\gamma$=1.2 the accretion disk is not formed in the system. Numerical results show that for case of $\gamma$=1.2 the 2D and 3D solutions are different. We discuss the spiral-shaped shock waves obtained in numerical models. It is shown that these shocks are not intrinsic spirals and are caused by collisions of the gaseous flows in the system.
Citation:
D. V. Bisikalo, A. A. Boyarchuk, O. A. Kuznetsov, D. Molteni, V. M. Chechetkin, “Comparison of 2d and 3d Models of Flow Structure in Semidetached Binaries”, Keldysh Institute preprints, 1998, 041
Linking options:
https://www.mathnet.ru/eng/ipmp1355 https://www.mathnet.ru/eng/ipmp/y1998/p41
|
|