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High Energy Pulsars: Pulses and Populations

Published online by Cambridge University Press:  12 April 2016

Roger W. Romani
Roger W. Romani*
Affiliation:
Department of Physics, Stanford University, CA [email protected]
*
1Alfred P. Sloan

Abstract

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Recent X-ray and γ-ray observations have detected a number of isolated spin-powered pulsars. Studies of the pulse profiles of these objects are providing a useful guide to the site of the high energy emission. The γ-ray pulses, which are closely tied to the primary population of radiating particles, seem to be an especially useful discriminant between pulsar models. With an understanding of how the pulsar luminosity and beaming factors evolve with spin parameters, pulsar population syntheses can also be used to check the predictions of high energy emission models. In turn, comparison with γ-ray sky surveys constrains the properties of the young pulsar population.

Type
Part 5 High Energy Phenomena
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 331 - 338
Copyright
Copyright © Astronomical Society of the Pacific 1996

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