Dynamic evolution of a quasi-spherical general polytropic magnetofluid with self-gravity

DOI10.1007/S10509-008-9807-6zbMath1145.85307arXiv0804.2889OpenAlexW2065819392MaRDI QIDQ944527

Yu-Qing Lou, Wei Gang Wang

Publication date: 17 September 2008

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0804.2889

zbMATH Keywords

MagnetohydrodynamicsStars: neutronClusters of galaxiesStars: formationStars: winds, outflowsSupernovae: general

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (1)

Dynamic evolution model of isothermal voids and shocks

Cites Work

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• Supersonic flow and shock waves. Reprint of the ed. published by Interscience Publishers, New York
• Self-similar dynamics of a magnetized polytropic gas
• Topological analysis of chaotic dynamical systems
• Self-Similar Solutions as Intermediate Asymptotics

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