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.
出处
《天文学进展》
CSCD
北大核心
1995年第1期30-38,共9页
Progress In Astronomy
基金
国家自然科学基金
关键词
Γ射线源
暴源
宇宙飞行器
BATSE
Gammar rays
bursts-Gammar rays
observations-space vehicle
