摘要
对于超新星遗迹MSH 15-56和CTA 1,本文较详细地公布了由爱因斯坦卫星得到的X射线观测资料.根据这些资料,导出其物理特性,推导和预言其射电流量,并与前人的射电观测进行了比较.
This paper gives the observational data of MSH b-56 and CTA 1 from the Einstein satellite in detail. According to these data, some physical parameters or characteristics of MSH 15-56 and CTA 1 are derived and discussed. The derived radio flux is compared with that observed before.
基金
国家自然科学基金
