从活跃星系1H 0707-495中的铁K和L过渡的宽线辐射
A C Fabian1, A Zoghbi, R R Ross
1Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK. acf@ast.cam.ac.uk
Nature
|May 30, 2009
概括
在狭窄的赛弗特1星系1H 0707-495中检测到的宽铁K和L线表明,旋转黑洞事件视界附近的辐射. 这一发现提供了接近超大质量黑洞的相对论效应的证据.
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
- 黑洞物理学 黑洞物理学
背景情况:
- 在对黑洞旋转敏感的增长系统中观察到广泛的铁K线辐射.
- 铁L线排放预计具有高铁丰富性,但往往被掩盖.
- 西弗特星系是由超大质量黑洞驱动的活跃星系核.
研究的目的:
- 为了研究狭线赛弗特1星系1H 0707-495.5的光谱和时间特性.
- 为了寻找铁K和铁L排放线.
- 探测超大质量黑洞事件地平线附近的区域.
主要方法:
- 对X射线数据进行光谱分析,以识别铁K和L排放线.
- 定时分析用于测量直接和反射X射线辐射之间的反响滞后.
- 建模相对论效应以解释线路配置文件和定时信号.
主要成果:
- 在1H0707-495.5中检测到明亮的铁K和铁L排放线.
- 测量连续和反射辐射之间的~30秒的反响滞后.
- 观察到的延迟与黑洞光分钟内物质的辐射一致.
结论:
- 综合的光谱和时间数据强烈表明,来自非常接近事件视界的物质的辐射.
- 这些发现为1H 0707-495.5中的一个快速旋转的大质量黑洞提供了证据.
- 这项研究表明了光谱和时间分析在探测极端黑洞环境中的力量.
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