A hydrodynamic model for an ideal polytropic gas rotating around a gra
vitating center is considered. Various stationary cylindrically symmet
ric analytical solutions are obtained, describing possible configurati
ons of the material. The possibility of constructing solutions describ
ing disk-like configurations of material in any shape is demonstrated.
A method for use of the three-dimensional stationary solutions obtain
ed as input data for numerical modeling of accretion disk processes in
the two-dimensional approximation is proposed. Numerical calculations
supporting the results of the theoretical studies are presented.