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X射线双星系统的探测
The X-ray binary system in the EP era
【摘要】 搜寻X射线双星并建立大规模样本是解决众多科学问题(如"银河系中有多少黑洞X射线双星?黑洞和中子星之间有无质量间隙?球状星团中有无黑洞?"等)的基础.爱因斯坦探针卫星拥有更灵敏的探测能力,将在运行的几年之中,预计可以发现一批新的中子星和黑洞X射线双星,研究其空间和动力学质量分布成为解决上述问题的关键.
【Abstract】 Searching for X-ray binaries and establishing a large sample are the foundation of answering many scientific problems,such as, how many BH X-ray binaries are there within our Milky Way galaxy? Does there exist a real gap between the mass distribution of neutron stars and black holes? Is there any black hole system within globular clusters? The planned mission Einstein Probe(EP) has a much better sensitivity compared to the past missions, so it is expected to discover many new X-ray binary systems over its operating period, which will play a key role in helping solve the problems above then.
- 【文献出处】 中国科学:物理学 力学 天文学 ,Scientia Sinica(Physica,Mechanica & Astronomica) , 编辑部邮箱 ,2018年03期
- 【分类号】P153;P172.2
- 【被引频次】2
- 【下载频次】207