On the initial phase of interaction between expanding stellar envelopes and surrounding medium

DOI10.1007/BF00653506zbMath0593.76075OpenAlexW1974694458MaRDI QIDQ1076575

D. K. Nadyozhin

Publication date: 1985

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

Full work available at URL: https://doi.org/10.1007/bf00653506

zbMATH Keywords

shock wavesimilarity solutioncontact discontinuityRayleigh- Taylor instabilitycharacteristics of the similarity solutioncircumstellar medium of a stellar envelopedensity laws of an expanding envelopeexpanding envelopeinitial stages of decelerationinternal shock waveoverall flow patternspherical-symmetric adiabatic hydrodynamicsstellar material

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Galactic and stellar dynamics (85A05) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

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