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A Joint Model for Radio and γ-ray Emission from Pulsars

Published online by Cambridge University Press:  26 May 2016

G. J. Qiao ,
K. J. Lee ,
H. G. Wang  and
R. X. Xu
G. J. Qiao
Affiliation:
Astronomy Department, Peking University, Beijing 100871, P.R. China
K. J. Lee
Affiliation:
Astronomy Department, Peking University, Beijing 100871, P.R. China
H. G. Wang
Affiliation:
Astronomy Department, Peking University, Beijing 100871, P.R. China
R. X. Xu
Affiliation:
Astronomy Department, Peking University, Beijing 100871, P.R. China

Abstract

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Although pulsars can radiate electromagnetic wave from radio to gamma ray bands, we still have no a united model to understand the multi-band emission. In this paper the effort for a joint model is presented. The inverse Compton scattering (ICS) and a second acceleration process near the null surface are involved to account for the radio and the gama-ray emission, respectively. Various kind of pulse profiles and other observational properties can be reproduced.

Type
Part 5 Pulsars and Other Neutron Stars
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 167 - 170
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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