Self-similar motions of self-gravitating gas in stars

DOI10.1007/BF01085040zbMath0606.76059MaRDI QIDQ1084995

Oleg I. Bogoyavlenskij

Publication date: 1986

Published in: Journal of Soviet Mathematics (Search for Journal in Brave)

zbMATH Keywords

shock wavesimilarity solutionsideal gasthree dimensionalhomogeneous cosmological modelsradial oscillationsadiabatic and similarity indexescomplete qualitative investigationsimilarity accretionspherically-symmetric self-gravitating gas configurationstellar burst

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Gas dynamics (general theory) (76N15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• Propagation of spherical shock waves in stars
• The instability of liquid surfaces when accelerated in a direction perpendicular to their planes. I
• Unnamed Item

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