Abstract
The results of two-dimensional, non-adiabatic gas dynamical simulations of gas flows in symbiotic stars are presented. It is shown that for a binary system with components that do not fill their Roche lobes, the structure of the gaseous stream is determined not only by the flow from the vicinity of the inner Lagrangian point, but also by the flow of matter caused by the orbital motion of the accretor through the gas of the stellar wind.
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