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A self-similar flow in generalised roche model with radiation heat flux, II

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Abstract

Self-similar flows of a gas moving under the gravitational attraction of a central body of fixed mass behind a spherical shock wave and propagating in a non-uniform atmosphere at rest, taking radiation heat flux into consideration, are investigated. The total energy of the wave between the shock front and inner expanding surface is taken to be time-dependent.

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Authors and Affiliations

  1. Department of Mathematics, S.G.R. Postgraduate College, Dobhi, Jaunpur, India

    J. B. Singh & P. R. Vishwakarma

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  1. J. B. Singh
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  2. P. R. Vishwakarma
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Singh, J.B., Vishwakarma, P.R. A self-similar flow in generalised roche model with radiation heat flux, II. Astrophys Space Sci 90, 161–169 (1983). https://doi.org/10.1007/BF00651557

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  • DOI: https://doi.org/10.1007/BF00651557

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