黑洞候选物XTE J1118+48080中的相关快速X射线和光学变异性
G Kanbach1, C Straubmeier, H C Spruit
1Max-Planck-Institut für Extraterrestrische Physik, Postfach 1317, 85741 Garching, Germany.
Nature
|November 9, 2001
概括
黑洞的积累可以通过新的X射线和光学数据更好地理解. 对XTE J1118+480的观测表明光学光源来自于循环同步子辐射,这表明外流缓慢.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- 黑洞积聚物理 黑洞积聚物理
背景情况:
- 黑洞是通过恒星伴侣的气体积累来观察的.
- 标准的薄增积盘模型无法解释观察到的X射线变化和流出.
研究的目的:
- 为了研究黑洞积聚系统的物理条件.
- 解释短暂源中X射线和光学辐射之间的令人费解的相关性.
主要方法:
- 同时进行高时间分辨率的X射线和光学观测.
- 暂时源XTE J1118+480.0.的分析
主要成果:
- 观察到X射线和光学辐射之间的强烈,令人费解的相关性.
- 光学辐射在X射线增加后突然上升,先后出现下降.
- 观察到的时间与重新处理的X射线发射模型不一致.
结论:
- 光学辐射很可能源于黑洞附近的循环同步子辐射.
- 时间依赖性表明缓慢 (<0.1c),磁性控制的外流.
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