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


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).


Atmosphere Nonlinear Function Optical Depth Transfer Equation Coherent Scattering 
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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  1. Busbridge, I. W.: 1953,Monthly Notices Roy. Astron. Soc. 113, 52.Google Scholar
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  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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