摘要
在A－S模型的基础上，讨论了脉冲星的γ射线辐射机制．考虑到偶极和四极场的作用后，给出了脉冲星要成为γ射线脉冲星的判据．据此判据计算了13颗可能成为γ射线脉冲星的光度和流量．
Based on A-S model, the mechanism of γ- ray emission of pulsars is discussed.After considering both dipole and quadrupole magnetic fields, the criterion of radio pulsars as a γ-ray pulsars is presented. Accroding to the criterion, the luminosities and fluxes of thirteen pulsars which are possible γ-ray pulsars are calcutated.
出处
《北京师范大学学报（自然科学版）》
CAS
CSCD
北大核心
1997年第2期188-193,共6页
Journal of Beijing Normal University(Natural Science)
基金
国家自然科学基金!19573006
