О трехмерном численном моделировании гидродинамической и гравитационной неустойчивости протопланетного диска

DOI10.20948/MM-2020-10-08zbMath1455.83014OpenAlexW3085447551MaRDI QIDQ5141827

L. G. Strakhovskaya

Publication date: 19 December 2020

Published in: Математическое моделирование (Search for Journal in Brave)

Full work available at URL: http://mathnet.ru/eng/mm4226

zbMATH Keywords

fragmentationshear flowgravitational instabilityproto-planet disk

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Cites Work

• Unnamed Item
• Stability and transition in shear flows
• Introduction to Hydrodynamic Stability
• On the nature of the core-envelope boundary layer in a slowly rotating star

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