伽玛射线暴源的新分布:BATSE的观测结果  

New Distributions and of Gamma-ray Busters:the BATSE Observational Results

作　　者：徐达维[1] 史天一[1] 

机构地区：[1]北京师范大学物理系,北京100875

出　　处：《天文学进展》1995年第1期30-38,共9页Progress In Astronomy

基　　金：国家自然科学基金

摘　　要：介绍了康普顿γ射线天文台上BATSE有关暴源分布观测的新发现。这一发现对80年代以前所普遍接受的γ射线暴起源于银盘内中子星的模型提出了严重挑战，并阐明了几种以BATSE结果为基础的暴源分布模型。The new discovery of the burster distribution obtained from BATSE on Compton GRO is introduced in this paper. It is faced on a serious challenge by the discovery that Gammaray bursts originate from neutron stars in galactic disk, which was generally accepted before the end of 80s. Based on the BATSE results, some burster distribution models are explained.

关 键 词：Γ射线源 暴源 宇宙飞行器 BATSE 

分 类 号：P172.3[天文地球—天文学]