Astrophysics and Space Science

, Volume 32, Issue 2, pp 375–377 | Cite as

Wave zone structure of NP 0532 and infrared radiation excess of Crab Nebula

  • V. V. Usov
Article

Abstract

At the distancer≳1015 cm from NP 0532 the plasma concentration decreases so that the intense low-frequency wave (ν=30 Hz) can propagate. The interaction of this wave with the electrons ejected from the pulsar should result in the IR radiation withFν∼102 fu at λ∼10 μ. This flux is the order of the excess IR radiation from the Crab Nebula.

Keywords

Radiation Plasma Concentration Infrared Radiation Zone Structure Wave Zone 

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References

  1. Aitken, D. K. and Polden, P. G.: 1971a,Nature Phys. Sci. 233, 45.Google Scholar
  2. Aitken, D. K. and Polden, P. G.: 1971b,Nature Phys. Sci. 234, 72.Google Scholar
  3. Kaw, P. and Dawson, J.: 1970,Phys. Fluids 13, 472.Google Scholar
  4. Michel, F. C.: 1969,Astrophys. J. 158, 727.Google Scholar
  5. Ozernoy, L. M. and Usov, V. V.: 1973,Astrophys. Letters 13, 151.Google Scholar
  6. Pacini, F.: 1970, Preprint CRSR 366.Google Scholar
  7. Shklovsky, I. S.: 1968,Supernovae, John Wiley and Sons, New York and London.Google Scholar
  8. Shklovsky, I. S.: 1970,Astrophys. J. 159, L77.Google Scholar

Copyright information

© D. Reidel Publishing Company 1975

Authors and Affiliations

  • V. V. Usov
    • 1
  1. 1.Space Research InstituteMoscowUSSR

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