Statistical study of high energy radiation from rotation-powered pulsars

被引：0
作者：
Zheng, GS [1 ]
Cheng, KS
Zhang, L
机构：
[1] Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China
[2] Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China
来源：
SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY | 2000年 / 43卷 / 02期
关键词：
gamma rays; theory-pulsars; general-stars; neutron-stars; statistics;
D O I：
10.1007/BF02876043
中图分类号：
O29 [应用数学];
学科分类号：
070104 ;
摘要：
Based on our self-consistent outer gap model for high energy emission from the rotation-powered pulsars, we study the statistical properties of X-ray and gamma-ray emission from the rotation-powered pulsars, and other statistical properties (e.g. diffuse gamma-ray background and unidentified gamma-ray point sources) related to gamma-ray pulsars in our Galaxy and nearby galaxies are also considered.
引用
收藏
页码：171 / 179
页数：9
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