在X射线二进制星 MAXI J1820+070 中的黑洞自转轨道错位
Juri Poutanen1,2,3, Alexandra Veledina1,2,3, Andrei V Berdyugin1
1Department of Physics and Astronomy, FI-20014 University of Turku, Finland.
概括
黑洞旋转轨道错位在X射线二进制系统中可能超过40°. 在MAXI J1820+070中观察到的这种显著的错位可能会对X射线数据中的黑洞质量和自旋测量产生偏差.
科学领域:
- 天体物理学
- 射线天文学
- 黑洞物理
背景情况:
- 在X射线二进制星系中,黑洞的观测特征受质量,旋转,积累率和旋转轨道错位的影响.
- 了解这些参数对于准确的黑洞描述至关重要.
研究的目的:
- 为了限制黑洞X射线二进制 MAXI J1820+070 的旋转轨道错位角度.
- 调查这种误差对黑洞参数测量的影响.
主要方法:
- 用光学极度测量来确定二进制轨道位置的角度.
- 结合现有的喷气方向 (追踪黑洞旋转) 和轨道倾斜的数据.
主要成果:
- 在MAXI J1820+070中确定了旋转轨道错位角的下限为40°.
- 这种显著的错位表明二进制进化或黑洞形成的起源.
结论:
- 在黑洞X射线双星中存在巨大的旋转轨道错位.
- 这种错位可以引入来自X射线观测的黑洞质量和自旋测量偏差.
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