A numerical model related to an astrophysical problem

DOI10.1016/0096-3003(89)90037-4zbMath0662.76094OpenAlexW2053997778MaRDI QIDQ1114524

A. Zaretti, Ulderico Bulgarelli, Maria Mercede Cerimele

Publication date: 1989

Published in: Applied Mathematics and Computation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0096-3003(89)90037-4

zbMATH Keywords

numerical methodNavier-Stokes equationscompressible viscous fluidsmotion of stars in a galaxy

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Existence, uniqueness, and regularity theory for compressible fluids and gas dynamics (76N10) Basic methods in fluid mechanics (76M99)

Cites Work

• A numerical method for a mathematical model in gravitational hydrodynamics
• Pressure method for the numerical solution of transient, compressible fluid flows
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