相关实验视频
Updated: Jul 11, 2026

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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
发现一个发射高能马射线的持久微类星体
1Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, E-08028 Barcelona, Spain. Departamento de Fisica, Escuela Politecnica Superior, Universidad de Jaen, Calle Virgen de la Cabeza 2, E-23071 Jaen, Spain. Max Planck.
概括
研究人员发现了LS 5039,一个新的微夸星系统,它显示了持续的相对论等离子体射出. 这个微量子星可能与马射线源相关,这是首次在高能马射线中检测到这样的系统.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- X射线天文学X射线天文学
背景情况:
- 微量子星是恒星X射线二进制星体,类似于银河系外量子星.
- 在银河系中发现的微量子星数不多.
- 在高能马射线中没有检测到以前识别的微类星体.
研究的目的:
- 报道发现了一个新的微类星系,LS 5039.
- 为了调查LS 5039与马射线源的潜在关联.
主要方法:
- 对X射线二进制系统的观察.
- 分析来自COMPTON - 玛射线观测站卫星的数据.
- 确定相对论等离子体射出.
主要成果:
- LS 5039被确定为一个微夸星系统.
- 从LS 5039.9观察到相对论等离子体的明显持续喷射.
- LS 5039与能量马射线实验望远镜 (EGRET) 马射线源的潜在关联.
结论:
- LS 5039代表了微类星研究中的一个重大发现.
- 来自LS 5039的高能马射线的检测对于微类星体来说是前所未有的.
- LS 5039提供了一个独特的实验室,用于研究恒星系统中的相对论等离子体过程.
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