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To explain Crab pulsar emission by ICS Model

Published online by Cambridge University Press:  12 April 2016

J.L. Han ,
B. Zhang ,
G.J. Giao  and
R.X. Xu
J.L. Han
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100080, China
B. Zhang
Affiliation:
Department of Geophysics, Peking University, Beijing 100871, China
G.J. Giao
Affiliation:
Department of Geophysics, Peking University, Beijing 100871, China
R.X. Xu
Affiliation:
Department of Geophysics, Peking University, Beijing 100871, China

Abstract

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Primary results of our recent work show that radio, infrared and optical, X-ray and γ-ray emission of Crab pulsar might be explained by Inverse Compton Scattering (ICS) mechanism.

Type
Part 3 Radio Emission Processes
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 183 - 184
Copyright
Copyright © Astronomical Society of the Pacific 1996

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