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 sta...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.展开更多
基金This work was partially supported by RGC grant of Hong Kong Government and Natural Science Foundation of Yunnan Province.
文摘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.
