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Summary-Introduction

Published online by Cambridge University Press:  19 March 2018

E. Schatzman
E. Schatzman*
Affiliation:
Institut d'Astrophysique - Paris

Extract

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There is astrophysical evidence for the existence of shocks propagating in regions of variable density. We have therefore the choice of discussing first the physics of shocks in a variable density atmosphere, or the astrophysical phenomena. Following Kaplan's preliminary report, we shall describe first the astrophysical facts, for the reader to be able to understand the connection of the physics with the astrophysics.

Information

Type
Part III. Spherically-Symmetric Motions in Stellar Atmospheres
Information
Symposium - International Astronomical Union , Volume 12: Aerodynamic Phenomena in Stellar Atmospheres , 1960, pp. 209 - 226
Copyright
Copyright © Italian physical society 1960 

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