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Keldysh Institute preprints, 2025 044, 34 pp. (Mi ipmp3342)

Simulation of proto-planetary disk evolution under condition of axial symmetry

E. A. Zabrodina, L. A. Pliner


Abstract: On the base of numerical calculations quasi-stationary gas-dynamic processes in proto-planetary cloud are investigated. In the frame of 2D Godunov’s method some additions are proposed for more accurate account of gravitational and centrifugal forces.

Keywords: proto-planetary disk, gravity, rotation.



© Steklov Math. Inst. of RAS, 2026