Re-discussion, from the Wiewpoint of Aerodynamics. Remarks on Steady Perfect Fluid Flow with Spherical Symmetry

H. Liepmann; P. Germain

doi:10.1017/S0074180900104498

Re-discussion, from the Wiewpoint of Aerodynamics. Remarks on Steady Perfect Fluid Flow with Spherical Symmetry

Published online by Cambridge University Press: 19 March 2018

H. Liepmann and

P. Germain

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P. Germain: Affiliation:
Institute Henry Poincaré - Paris

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As discussed by DEUTSCH, the following gas-dynamical problem arises in the study of a stellar atmosphere: find a steady outward flow, originating from a star, which is compatible with the interstellar medium. In what follows, spherical symmetry will be assumed; moreover, the gas will be considered as a perfect gas with constant specific heats.

Type: Part III. Spherically-Symmetric Motions in Stellar Atmospheres
Information: Symposium - International Astronomical Union , Volume 12: Aerodynamic Phenomena in Stellar Atmospheres , 1960 , pp. 296 - 300

DOI: https://doi.org/10.1017/S0074180900104498 [Opens in a new window]

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Re-discussion, from the Wiewpoint of Aerodynamics. Remarks on Steady Perfect Fluid Flow with Spherical Symmetry

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