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Radiation from Pulsars

Published online by Cambridge University Press:  07 February 2017

I. Lerche
I. Lerche*
Affiliation:
Enrico Fermi Institute and Department of Physics, University of Chicago, Chicago, Ill., U.S.A.

Abstract

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We suggest that an oscillating interface, carrying a steady current between a rotating, radiating, magnetic dipole and an external plasma is the source of pulsar radiation produced over a broad band of high frequencies (108–1018 Hz). The efficiency of the radiation mechanism is so high that the oscillation energy goes mainly into radiation in each cycle of the oscillation.

Type
Session 8
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 449 - 454
Copyright
Copyright © Reidel 1971 

References

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