A joint model for radio and γ-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：
HIGH ENERGY PROCESSES AND PHENOMENA IN ASTROPHYSICS | 2003年 / 214期
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：
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.
引用
收藏
页码：167 / 170
页数：4
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