相关实验视频
Updated: Jul 27, 2026

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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
来自微类星 LS I +61 303 的可变非常高能马射线辐射
1Universität Würzburg, D-97074 Würzburg, Germany.
概括
我们检测到微类星LS I 61 + 303的可变马射线辐射,表明周期性活动. 这一发现为相对论喷流和宇宙射线起源的物理学提供了洞察力.
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
- 马射线天文学 马射线天文学
背景情况:
- 微量子星是发射相对论喷射的二进制系统,对于研究宇宙射线和喷射物理学至关重要.
- 了解微类星体排放有助于解开高能天体物理现象.
研究的目的:
- 报告从微类星 LS I 61 + 303.3 中检测到可变的马射线辐射.
- 为了研究微量子星中的玛射线辐射的周期性和轨道调制.
主要方法:
- 使用玛射线望远镜检测100千兆电子伏特以上的辐射.
- 分析了微类星 LS I 61 + 303 的六个轨道周期.
- 将玛射线发射模式与二进制星系的轨道相相关联.
主要成果:
- 来自LS I 61 + 303的100GeV以上的可变马射线辐射的检测.
- 在马射线检测中观察到的周期性,与特定的轨道相相一致.
- 最强的马射线发射在最近的恒星接近时没有被检测到,这表明轨道调制.
结论:
- 小类星 LS I 61 + 303 呈现周期性马射线发射.
- 轨道调制显著影响观察到的发射或吸收过程.
- 这些发现有助于理解微类星体物理及其作为宇宙射线源的作用.
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