扩展硬X射线发射在银河系的内部几个帕塞克
Kerstin Perez1, Charles J Hailey2, Franz E Bauer3
11] Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, Room 1027, New York, New York 10027, USA [2] Haverford College, 370 Lancaster Avenue, KINSC L109, Haverford, Pennsylvania 19041, USA.
Nature
|May 1, 2015
概括
天文学家在银河系中心发现了一种明显的硬X射线辐射. 这一发现挑战了目前在射手座A*附近的恒星进化和宇宙射线产生模型.
科学领域:
- 天体物理学 天体物理学
- 高能天文学 高能天文学
- 银河系中心研究研究
背景情况:
- 银河系中心包含一个令人费解的年轻群体,巨大的恒星附近的射手座A*.
- 以前的研究已经确定软X射线来源主要是白矮星的积累.
- 对分散的硬X射线辐射的观察受到仪器分辨率的限制.
研究的目的:
- 为了研究银河系中心内部的硬X射线辐射,并提高空间分辨率.
- 为了描述这种硬X射线组件的性质和起源.
主要方法:
- 在20-40千电子伏特能量范围内利用分分钟以下的分辨率成像.
- 分析了银河中心中央4 × 8帕塞克内的分散硬X射线辐射.
主要成果:
- 在中央4 × 8帕塞克中报告了明显的硬X射线组件的存在.
- 观察到,这种硬X射线辐射在银河系中心的峰值比软X射线源更为明显.
结论:
- 这些发现表明,可能包括一个更大规模的白矮星,低质量X射线二进制星,毫秒脉冲星或粒子外流.
- 这些解释对现有的恒星进化,双星形成和银河系中心宇宙射线产生理论提出了重大挑战.
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