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Astrophysics

Title: Physical processes in pulsar magnetospheres and non-thermal high-frequency emission

Authors: Vladimir V. Usov
(Submitted on 9 Dec 1996)
Abstract: The energy source of a pulsar's non-thermal emission is the rotational energy loss of the neutron star. The rotational energy of the neutron star is transformed into the pulsar radiation by a long sequence of processes. The processes of this sequence are discussed.
Comments: 8 pages, latex, no figures. To be published in the Proceedings of the IAU Colloquium No 160, Pulsars: Problems and Progress, Sydney, 8-12 January 1996 (invited paper)
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/9612078v1

Submission history

From: Mail [view email]
[v1] Mon, 9 Dec 1996 10:26:20 GMT (10kb)
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