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The Radiation Mechanism in Pulsars

Published online by Cambridge University Press:  07 February 2017

F. G. Smith
F. G. Smith*
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, U.K.

Abstract

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The properties of the radio pulses from pulsars are described. The formation of pulses seems to be a geometric phenomenon, for which the beaming due to relativistic motion of the source is the only candidate at present. Values of the volume emissivity and surface flux density indicate that all the particles near the source must have relativistic energies.

Type
Session 8
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 431 - 440
Copyright
Copyright © Reidel 1971 

References

Smith, F. G.: 1970, Monthly Notices Roy. Astron. Soc. 149, 1.Google Scholar