解析的原子线显示了两个超光X射线源的外流
Ciro Pinto1, Matthew J Middleton1, Andrew C Fabian1
1Institute of Astronomy, Cambridge University, Madingley Road, Cambridge CB3 0HA, UK.
Nature
|April 28, 2016
概括
超发光的X射线源呈现出快速外流的风,由蓝移的X射线吸收线证明. 这些强大的风围绕着紧的物体,
科学领域:
- 天体物理学
- 高能天体物理学
- 射线天文学
背景情况:
- 超发光X射线源 (ULX) 是银河系外的点光源,其发光度超过3 × 10^39 ergs/sec.
- ULX是通过对紧物体的积累获得动力,可能是中子星或恒星质量到中等质量的黑洞.
- 之前的分析缺乏识别光谱线的能量分辨率,阻碍了积累流的研究.
研究的目的:
- 使用高分辨率X射线光谱分析ULX中的积累流.
- 识别和描述ULX中的光谱特征,以确定紧物体及其周围的性质.
主要方法:
- 两个ULX的高分辨率X射线光谱分析:NGC 1313X-1和NGC 5408X-1.
- 在X射线光谱中检测和显著性的排放和吸收线.
主要成果:
- 检测到高电离铁,氧气和的X射线.
- 显著检测到蓝色移动的吸收线,表明快速流出的气体.
- 排放线源于缓慢移动的气体,而吸收线源于大约0.2倍光速的气体外流.
结论:
- NGC 1313X-1和NGC 5408X-1中的紧物体被强烈的风环绕.
- 观测到的风的流出速度约为0.2c,与超大质量黑洞和超大质量黑洞的模型相一致.
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