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Distance of the Far Galaxies and Scattering of the Photons in the Space

  • M. Missana
Part of the Astrophysics and Space Science Library book series (ASSL, volume 121)

Abstract

From the theory of the radiative transfer, including the scattering of the light and the Compton effect, it can be deduced that the intensity of the far astrophysical objects decreases approximatively as 1/R3.

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References

  1. Allen C.W.:1973,Astrophysical Quantities,The Athlone Press, London, p.293.Google Scholar
  2. Eddington S.A.:1926,The Internal Constitution of the Stars, Cambridge University Press,p.371.Google Scholar
  3. Missana M.:1977,Astrophys.Space Sci.50,409.ADSCrossRefGoogle Scholar
  4. Missana M.:1979,Astrophys.Space Sci.61,277.ADSCrossRefGoogle Scholar
  5. Missana M.:1984,Atti XXV Riunione Società Astonom.Ital. , Suppl. al Vol.55°-N°1-1984,p.221.Google Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1986

Authors and Affiliations

  • M. Missana
    • 1
  1. 1.Osservatorio Astronomico di BreraMilanoItaly

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