The emergence of a spherical magnetogasdynamic shock wave at the surface of a star

DOI10.1007/BF00651300zbMath0514.76067MaRDI QIDQ1051531

R. C. Srivastava

Publication date: 1983

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

zbMATH Keywords

flow behind isothermalmagnetogasdynamic shock wave originating in stellar interiorproduct solution of McVittiesurfaces of star

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar dynamics (85A05)

Related Items (1)

Jump conditions for shock waves on the surface of a star

Cites Work

• The isothermal expansion of a gas cloud into a non-uniform atmosphere
• On the propagation of shock waves through regions of non-uniform area or flow
• On the problem of a shock wave arriving at the edge of a gas
• Equatorial propagation of axisymmetric magnetohydrodynamic shocks
• Spherically symmetric solutions of the equations of gas dynamics

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