An isothermal shock wave in a perfectly-conducting and non-homogeneous stellar interior

DOI10.1007/BF00648994zbMath0516.76053MaRDI QIDQ1052903

B. G. Verma, J. P. Vishwakarma, Vishnu Sharan

Publication date: 1982

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

zbMATH Keywords

initial densitymagnetogasdynamicexact analytic self-similar solutionssingular surface behindstellar explosionszero-temperature gradient

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

• Unnamed Item
• A model of flare-produced magneto radiative shock with increasing energy
• Propagation of spherical shock waves in stars
• On the problem of a shock wave arriving at the edge of a gas

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