相关实验视频
Updated: May 31, 2026

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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
一个极其明亮的泛色爆发来自一个遥远的银河系的核
A J Levan1, N R Tanvir, S B Cenko
1Department of Physics, University of Warwick, Coventry, UK. a.j.levan@warwick.ac.uk
概括
天文学家观察到一个独特的,极其明亮的宇宙事件,具有持久的高能发射,与以前见过的不同. 这种强大的爆发可能源于一个罕见的机制,涉及银河系中心的大型黑洞.
科学领域:
- 高能天体物理学 高能天体物理学
- 多波长天文学多波长天文学
- 太空中的短暂物.
背景情况:
- 可变的X射线和马射线辐射意味着极端的宇宙过程.
- 斯威夫特卫星检测到马射线选择的短暂物.
研究的目的:
- 为了呈现一个独特的马射线短暂的多波长观测.
- 描述其电磁频谱和属性.
- 为了确定这种前所未有的现象的起源.
主要方法:
- 利用Swift卫星进行马射线检测.
- 在整个电磁频谱进行了多波长观测.
- 确定了事件在宿主星系中的位置.
主要成果:
- 检测到一种独特的马射线瞬态,具有异常明亮的广谱辐射.
- 将事件定位到一个恒星形成星系的中心,红移z = 0.3534.
- 观测到长时间的高能辐射远远超过典型的马射线爆发.
- 测量到的峰值亮度大约是明亮活跃星系核的100倍.
结论:
- 瞬态的特性与以前观察到的任何宇宙源都不同.
- 它与银河系核的关联表明,一个罕见的机制涉及中央大质量黑洞.
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