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来自超发光超软X射线源的相对论微子喷射
Ji-Feng Liu1,2, Yu Bai1, Song Wang1
1Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China.
Nature
|November 26, 2015
概括
天体物理学家观察到来自超光超软X射线源 (ULS) 的相对论喷射,挑战目前的喷射形成理论. 这种意想不到的发现表明, 超级积聚的黑洞可能是造成这些强大的外流的原因.
科学领域:
- 天体物理学
- 射线天文学
- 紧物体研究
背景情况:
- 这是一个关键的天体物理学难题.
- 微类星体表现出已建立的相对论喷气现象学.
- 超软的X射线来源通常不会产生相对论喷射,但有些人会显示低速度的外流.
研究的目的:
- 研究超光超软X射线源 (ULS) 中的相对论喷流的性质.
- 分析ULS M81ULS-1的光学光谱.
- 挑战和完善现有的相对论喷气形成理论.
主要方法:
- M81 ULS-1 的光学光谱
- 时间变量,蓝移 Hα 排放线的分析.
- 与已知的微类星相比,如SS 433.
主要成果:
- 来自M81 ULS-1的微粒子喷射中观察到的相对论速度 (17%的光速).
- 检测到时间变量,广泛的Hα发射线.
- 发现了与SS 433微准星相似的特性.
结论:
- 在ULS中存在相对论喷流挑战了正规的喷流形成理论.
- 这些发现表明ULS与具有光学厚度的黑洞之间存在潜在的联系.
- 这一发现为了解喷气式发射机制开辟了新的途径.
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