Statistical study of high energy radiation from rotation-powered pulsars  

作　　者：郑广生 张力 

出　　处：《Science China Mathematics》2000年第2期171-179,共9页中国科学：数学（英文版）

基　　金：This work was partially supported by RGC grant of Hong Kong Government and Natural Science Foundation of Yunnan Province.

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 y-ray emission from the rotation-powered pulsars, and other statistical properties (e.g. diffuse y-ray background and unidentified y-ray point sources) related to y-ray pulsars in our Galaxy and nearby galaxies are also considered.Based on our self-consistent outer gap model for high energy emission from the rotationpowered pulsars, we study the statistical properties of X-ray and y-ray emission from the rotation-powered pulsars, and other statistical properties (e.g. diffuse y-ray background and unidentified y-ray point sources) related to y-ray pulsars in our Galaxy and nearby galaxies are also considered

关 键 词：GAMMA RAYS theory-pulsars general-stars NEUTRON-STARS statistics. 

分 类 号：P145.8[天文地球—天体物理]