A mathematical solution for the formation of halo

DOI10.1007/BF00651583zbMath0545.76149OpenAlexW2035477633MaRDI QIDQ798227

N. E. Zubov

Publication date: 1984

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

Full work available at URL: https://doi.org/10.1007/bf00651583

zbMATH Keywords

magnetohydrodynamic equationsgravitational potentialdense astrophysical systemsformation of corona, envelope of supergiant or galactic halogeneral dispersion relation

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar dynamics (85A05)

Cites Work

• Collisionless Heating of the Solar-Wind Plasma. I. Theory of the Heating of Collisionless Plasma by Hydromagnetic Waves

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