Dv. Bisikalo et al., The effect of viscosity on the flow morphology in semidetached binary systems. Results of 3D simulations. II, ASTRON REP, 44(1), 2000, pp. 26-35
We present the results of three-dimensional simulations of matter flows in
semidetached binary systems with various viscosities. In low-viscosity syst
ems, the flow structure displays the same qualitative features as in high-v
iscosity computations. A self-consistent solution shows the absence of a sh
ack interaction between the stream flowing from the inner Lagrange point an
d the forming accretion disk (or hot spot) for any viscosity. (C) 2000 MAIK
"Nauka/Interperiodica".