摘要
基于对磁化中子星磁层中极相对论电子辐射机制和辐射输运性质的讨论，指出被观测到的硬γ射线可能来自于磁化中子星的逃逸同步曲率辐射光子．逃逸硬γ射线光子最有可能产生于光速柱面附近的一个区域．
ased on the discussions of emission mechanisms of extreme relativistic electrons and propagation properties of radiations in the magnetosphere of magnetized neutron stars, it is indicated that some hard gamma rays detected by energetic gamma ray telescopes would be the escaped synchrotron curvature photons from the magnetized neutron stars and possibly producted in an area nere the surface of light cylinders.
出处
《首都师范大学学报（自然科学版）》
1998年第1期27-30,共4页
Journal of Capital Normal University：Natural Science Edition
关键词
Gamma射线
同步曲率辐射
磁对产生
中子星
非热发射源
gamma rays,synchrotron curvature radiations,magnetic pair production,neutron stars,non thermal emission sources.
