摘要
本文以极冠模型为基础，计算了脉冲星γ射线辐射光度，指出对不同的脉冲星必须考虑辐射立体角和可见辐射区对观测光度的影响．考虑了这些观测效应后，计算的光度和观测值基本符合．预言了一些可能的γ射线脉冲星，并对其性质进行了研究．
Based on the polar cap model,the radiant luminosity of γ -ray pulsars is calculated in this paper.The authors point out that solid angle and visible emission region must be considered for radiant luminosity calculation. After considering these observational effects,the calculated luminosity of γ -ray pulsars is in agreement with observation.Furthermore,the character of some γ -ray pulsar candidatesis predicted in the paper.
基金
国家自然科学基金
中国科学院"九五"基础研究青年基金
