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A self-similar flow of self-gravitating gas behind a shock wave with radiation heat flux, I

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Abstract

Self-similar flows of self-gravitating gas behind the spherical shock wave propagating in a non-uniform atmosphere at rest, taking radiation heat flux into consideration, are investigated. The total energy of the wave is non-constant and can be made to vary slowly with time.

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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 of self-gravitating gas behind a shock wave with radiation heat flux, I. Astrophys Space Sci 90, 153–159 (1983). https://doi.org/10.1007/BF00651556

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  • DOI: https://doi.org/10.1007/BF00651556

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