Dependence of scaled vertically integrated density and radial and azimuthal disk velocities and the scaled angular momentum loss rate on radius in the case of isothermal disk (p = 0) of selected B0-type star for various radial viscosity profiles (various n) in a final stationary state of time-dependent models (the rapid drop of rotational velocity and the angular momentum loss rate in the outer disk region is a stationary jump, not a shock wave).