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Astrophysics and Space Science

, Volume 90, Issue 1, pp 153–159 | Cite as

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

  • J. B. Singh
  • P. R. Vishwakarma
Article

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.

Keywords

Radiation Atmosphere Heat Flux Shock Wave Total Energy 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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Copyright information

© D. Reidel Publishing Co. 1983

Authors and Affiliations

  • J. B. Singh
    • 1
  • P. R. Vishwakarma
    • 1
  1. 1.Department of MathematicsS.G.R. Postgraduate CollegeJaunpurIndia

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