与快速无线电爆发相关的密集磁性等离子体
Kiyoshi Masui1,2, Hsiu-Hsien Lin3, Jonathan Sievers4,5
1Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia V6T 1Z1, Canada.
Nature
|December 4, 2015
概括
快速无线电爆发 (FRB) 显示出显著的法拉第旋转,表明源附近的磁化. 这一发现支持了FRB起源的磁星模型,将其与中子星合并的场景区分开来.
科学领域:
- 天体物理学
- 宇宙学
- 无线电天文学
背景情况:
- 快速无线电爆发 (FRB) 是持续数毫秒的银河系外无线电短暂.
- 之前的FRB缺乏可检测的线性极化, 阻止法拉第旋转测量.
- 它们的散射尺度表明它们的宇宙距离.
研究的目的:
- 为了研究FRB 110523中的法拉第旋转.
- 确定FRB的源环境和来源.
主要方法:
- 对FRB110523的档案数据进行分析.
- 银河系和银河间分散度的建模.
- 对旋转量和散射特性进行评估.
主要成果:
- 在FRB110523中检测出显著的法拉第旋转.
- 在FRB源附近有磁化和散射的证据.
- 限制源红移最大值为0.5.
结论:
- 观察到的磁化和散射有利于像磁星这样的年轻,充满活力的源.
- 这挑战了涉及老中子恒星合并的模型.
- FRB环境很可能是密集的,可能在宿主星系内.
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