Radio and gamma-ray emission from pulsars

被引：0
|
作者：
Qiao, GJ [1 ]
Lee, KJ [1 ]
Wang, HG [1 ]
Xu, RX [1 ]
机构：
[1] Peking Univ, Dept Astron, Beijing 100871, Peoples R China
来源：
RADIO PULSARS, PROCEEDINGS | 2003年 / 302卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The radiation of pulsars have been observed for many years. A few pulsars are discovered to have both radio and gamma-ray emission. Many models oil pulsar radiation have been developed, but so far we are still lacking an elaborate model which call explain the emission from radio to gamma-rays in detail. In this paper we present a joint model for radio and gamma-ray emission, in which both the dominate emission mechanisms are inverse Compton scattering. The pulse profiles at radio and gamma-ray bands are reproduced for the Crab-like, Vela-like and Geminga-like pulsars, in good agreement with observations.
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页码：183 / 186
页数：4
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