一群发光的黑洞与隐藏的合并
Michael J Koss1,2, Laura Blecha3, Phillip Bernhard4
1Eureka Scientific Inc, Oakland, CA, USA. mike.koss@eurekasci.com.
Nature
|November 9, 2018
概括
超大质量黑洞的增长, 尤其是在后期阶段. 这项研究证实暗黑发光黑洞中存在大量晚期核聚变,支持聚变驱动的积累理论.
科学领域:
- 天体物理学
- 银河系的演变
- 黑洞积聚
背景情况:
- 大型星系的合并被认为是推动超大质量黑洞的增长.
- 这种联系的观察证据是混合的,一些研究表明存在相关性,而另一些则没有.
- 预计在合并过程中气体和尘埃的遮蔽会增加,在最后阶段达到顶峰.
研究的目的:
- 为了研究后期星系融合在超大质量黑洞成长中的作用.
- 为合并驱动黑洞积累的理论预测提供观测支持.
主要方法:
- 高分辨率红外成像硬X射线选择黑洞.
- 对宿主星系的融合阶段的分析.
- 与不活跃的星系进行比较, 恒星质量和恒星形成速度一致.
- 用水力学模拟来模拟合并过程.
主要成果:
- 与非活跃星系相比,在遮蔽的发光黑洞中发现了大量 (17.6%) 的后期核融合.
- 这与黑洞积聚在最后的合并阶段达到峰值的理论预测一致.
- 水力动力学模拟证实,富含气体的大型融合主体在这个阶段表现出最强的核融合.
结论:
- 晚期核聚变与隐蔽的超大质量黑洞有很强的联系.
- 这些发现支持这样一个假设:星系的合并,尤其是在它们的最后阶段,对于推动这些活跃黑洞的生长至关重要.
- 暗暗发光的黑洞代表了超大质量黑洞合并的原始群体.
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