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Radiating Regions in Pulsar Magnetospheres: From Theory to Observations and Back

Published online by Cambridge University Press:  12 April 2016

Vladimir V. Usov
Vladimir V. Usov*
Affiliation:
Department of Condensed-Matter Physics, Weizmann Institute of Science, Rehovot 76100, Israel

Abstract

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We discuss plausible locations of radiating regions in the magnetospheres of pulsars and argue that the mechanisms of pulsar radiation at different frequencies are closely connected with the locations of the radiating regions, especially in the radio range. If the region that is responsible for the bulk of the non-thermal radiation at some frequency is localized in the pulsar magnetosphere then the nature of this radiation will be either determined or, at least, restricted significantly.

Type
Part 6. Emission and Plasma Theory
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 417 - 420
Copyright
Copyright © Astronomical Society of the Pacific 2000

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