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伽玛射线暴源的新分布“BATSE的观测结果
引用本文:徐达维,史天一.伽玛射线暴源的新分布“BATSE的观测结果[J].天文学进展,1995,13(1):30-38.
作者姓名:徐达维  史天一
作者单位:北京师范大学物理系!北京,100875,北京师范大学物理系!北京,100875
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展。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BASE结果基础的暴源分布模型。

关 键 词:γ射线源  暴源  宇宙飞行器  BATSE

New Distributions and of Gamma-ray Busters:the BATSE Observational Results
Xu Dawei, Shi Tianyi.New Distributions and of Gamma-ray Busters:the BATSE Observational Results[J].Progress In Astronomy,1995,13(1):30-38.
Authors:Xu Dawei  Shi Tianyi
Abstract: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.
Keywords:Gammar rays  bursts-Gammar rays  observations-space vehicle
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