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Calculation of flow of stellar wind past an x-ray source - MaRDI portal

Calculation of flow of stellar wind past an x-ray source

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Publication:795640

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DOI10.1007/BF01090625zbMath0542.76062MaRDI QIDQ795640

K. V. Krasnobaev, R. A. Svunyaev

Publication date: 1983

Published in: Fluid Dynamics (Search for Journal in Brave)

zbMATH Keywords

binary star systems oscillatory accretion regime rate of accretion subsonic because of heating supersonic stellar wind x-ray sources

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (1)

Supersonic flow over energy-releasing sources

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