Astrophysics and Space Science

, Volume 192, Issue 1, pp 127–132 | Cite as

Solution of the equation of transfer for coherent scattering in an exponential atmosphere by Busbridge's method

  • T. K. Deb
  • S. Karanjai
Article

Abstract

A solution of the transfer equation for coherent scattering in stellar atmosphere with Planck's function as a nonlinear function of optical depth, viz.
$$B{\text{ }}_v (T) = b_0 + b_1 {\text{ }}e^{ - \beta \tau } $$
is obtained by the method developed by Busbridge (1953).

Keywords

Atmosphere Nonlinear Function Optical Depth Transfer Equation Coherent Scattering 

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References

  1. Busbridge, I. W.: 1953,Monthly Notices Roy. Astron. Soc. 113, 52.Google Scholar
  2. Chandrasekhar, S.: 1960,Radiative Transfer, Dover Publ., New York.Google Scholar
  3. Dasgupta, S. R.: 1977a,Astrophys. Space Sci. 50, 187.Google Scholar
  4. Dasgupta, S. R.: 1977b,Phys. Letters 64A, 342.Google Scholar
  5. Karanjai, S. and Deb, T. K.: 1991a,Astrophys. Space Sci. 178, 299.Google Scholar
  6. Karanjai, S. and Deb, T. K.: 1991b,Astrophys. Space Sci. 179, 89.Google Scholar
  7. Woolley, R. v. d. R. and Stibbs, D. W. N.: 1953,Outer Layers of a Star, Clarendon Press, Oxford.Google Scholar

Copyright information

© Kluwer Academic Publishers 1992

Authors and Affiliations

  • T. K. Deb
    • 1
  • S. Karanjai
    • 2
  1. 1.Department of TelecommunicationsSiliguriIndia
  2. 2.Department of MathematicsNorth Bengal UniversityIndia

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