Slaved Accretion Disk Model in Binaries with Precession of Mass-Losing Star

The results of 3D numerical simulation of mass transfer in semidetached binaries, mass-losing star of which has an own rotation, are presented. Vector of rotation of mass-losing star is assumed to precess in laboratory (inertial) frane. The 'slaved' model of accretion disk was confirmed for considered case.