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Formation of bipolar flow by the stellar wind embedded in molecular disk - MaRDI portal

Formation of bipolar flow by the stellar wind embedded in molecular disk

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Publication:1069402

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zbMath0583.76122MaRDI QIDQ1069402

Shiro Sakashita, Hitoshi Hanami, Masayuki Umemura

Publication date: 1985

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

zbMATH Keywords

similarity solution shock front equilibrium state density distribution bipolar flow isotropic stellar wind outflow in the bipolar sources rarefied interstellar gas rotating isothermal cloud shock envolope young star

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Galactic and stellar dynamics (85A05)

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