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A model for the energetic emission from pulsars

Published online by Cambridge University Press:  12 April 2016

Yu.E. Lyubarskii
Yu.E. Lyubarskii*
Affiliation:
Institute of Radio Astronomy, Krasnoznamyonnaya St.4, 310002, Kharkov, Ukraine

Abstract

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A current sheet separates, beyond the closed part of the pulsar magnetosphere, two half-spaces with oppositely directed magnetic fields. It is shown that reconnection in this sheet may provide a source for high-energy emission.

Type
Part 6. Emission and Plasma Theory
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 439 - 440
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Lyubarskii, Yu.E. 1996, A&A, 311, 172 Google Scholar
Zeleny, L.M., Krasnoselskikh, V.V., 1979, Astron.Zh. 56, 819.Google Scholar