Discovery and x-ray properties of GS 1124-683 (= Nova Muscae)
Discovery and x-ray properties of GS 1124-683 (= Nova Muscae)
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GS 1124-683（=新蝇）的发现和 X 射线特性
DOI：
10.1086/171614
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发表时间：
1992
期刊：
影响因子：
--
通讯作者：
K. Hayashida
中科院分区：
文献类型：
--
作者：
S. Kitamoto;H. Tsunemi;S. Miyamoto;K. Hayashida
1991年1月8日，银河上的全天监视器(ASM)发现了一颗明亮的X射线新星：GS 1124-683。观测到的光谱大致用一个由幂定律(硬X射线)和盘状黑体或黑体(软X射线)组成的两组分模型来描述。在它的上升阶段，随着温度和发射面积的增加，硬X射线成分首先出现，软X射线成分紧随其后
A bright X-ray nova: GS 1124-683 was discovered by the All Sky Monitor (ASM) on board Ginga on 1991 January 8. X-ray properties observed with the ASM from 1991 January 5 to the end of August are presented. The observed spectra were roughly described by a two-component model consisting of a power-law (a hard X-ray) and a disk-blackbody or a blackbody (a soft X-ray) component. In its rising phase, the hard X-ray component appeared first and the soft X-ray component followed with increase of the temperature and the emission area