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Updated: Mar 29, 2026

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来自光学和X射线明亮的恒星潮扰乱火焰ASASSN-14li的无线射流
S van Velzen1, G E Anderson2, N C Stone3
1Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, USA. sjoert@jhu.edu.
概括
天文学家检测到来自恒星的潮干扰事件 (TDE) 的无线电辐射, 这一发现意味着喷射可能在TDE中很常见,解释了为什么它们以前没有被检测到.
科学领域:
- 天文学与天体物理学
- 黑洞物理
- 高能天体物理学
背景情况:
- 超大质量黑洞 (SMBH) 可以带来潮破坏的恒星,
- 之前对热恒星潮扰乱火焰 (TDF) 的无线电观测没有产生确的检测结果.
- 寻找TDF的无线电对应物对于了解积累过程和喷气发射至关重要.
研究的目的:
- 报告第一个从热TDF的无线电发射的确检测.
- 调查这个无线电辐射的来源, 建议它来自一个新启动的喷气式飞机.
- 探索这种检测对TDF中喷气的共同性的影响.
主要方法:
- 一个特定的热TDF的多波长观测.
- 敏感的无线电跟踪观测以检测微弱的辐射.
- 观察到的特性与积累和喷气发射的理论模型的比较.
主要成果:
- 来自热TDF的可变无线电辐射的检测.
- 无线电发射的特性与恒星质量黑洞积聚状态中观察到的相似.
- 无线电观测的灵敏度明显高于之前的上限.
结论:
- 检测到的无线电辐射被解释为来自与TDF相关的新发射喷气机.
- 这表明喷气可能是所有TDF的共同现象.
- 无线电观测的增强灵敏度解释了为什么这些喷气可能在此之前没有被探测到.
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