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Self-similar flows behind a spherical radiation-driven shock wave, II

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Abstract

Self-similar flows, behind a radiation-driven shock wave, have been investigated in non-uniform atmosphere. The total energy content of the flow behind the shock increases due to the absorption of radiation and it is assumed to be time-dependent.

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References

  • Ranga Rao, M. P. and Ramana, B. V.: 1973,Int. J. Engng. Sc. 11, 1035.

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  • Singh, J. B.: 1981,Ind. J. Math. Soc. (in press).

  • Wilson, C. R. and Turcotte, D. L.: 1970,J. Fluid Mech. 43, 399.

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Author notes

  1. R. N. Lal Srivastava

    Present address: Department of Mathematics, D.A.V. College, Gorakhpur, U.P., India

Authors and Affiliations

  1. S.G.R. Postgraduate College, Dobhi, Jaunpur, (U.P.), India

    J. B. Singh & R. N. Lal Srivastava

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  1. J. B. Singh
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  2. R. N. Lal Srivastava
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Singh, J.B., Srivastava, R.N.L. Self-similar flows behind a spherical radiation-driven shock wave, II. Astrophys Space Sci 85, 437–441 (1982). https://doi.org/10.1007/BF00653465

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  • DOI: https://doi.org/10.1007/BF00653465

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