证据表明SgrA200年的X射线极化爆发
Frédéric Marin1, Eugene Churazov2,3, Ildar Khabibullin2,3,4
1Université de Strasbourg, CNRS, Observatoire Astronomique de Strasbourg, UMR 7550, Strasbourg, France. frederic.marin@astro.unistra.fr.
Nature
|June 21, 2023
概括
极化X射线观测揭示了射手座A*星系的过去活动
科学领域:
- 天体物理学
- 射线天文学
- 极极度测量
背景情况:
- 银河系的中心黑洞,射手座A* (Sgr A),目前处于静止状态.
- 周围气体的X射线反射可以探测Sgr A*过去的燃烧活动.
- 之前的观察表明了X射线发射的反射情况.
研究的目的:
- 调查来自银河系中心的极化X射线辐射.
- 确认反射场景并研究Sgr A*的历史亮度.
主要方法:
- 使用成像X射线极度测量探测器 (IXPE).
- 在Sgr A*附近的分子云的方向观察极化X射线发射.
主要成果:
- 测量极化度为31%±11%.
- 测量极化角度为-48°±11°.
- 结果与Sgr A*作为排放源是一致的.
结论:
- 这些发现支持Sgr A*的X射线反射模型.
- 暗示Sgr A*的X射线亮度与200年前的赛弗特星系略有相似.
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