一个持续活跃的快速无线电爆发源嵌入在一个膨胀的超新星残留物中
Chen-Hui Niu1, Di Li2, Yuan-Pei Yang3
1Institute of Astrophysics, Central China Normal University, Wuhan 430079, China.
Science bulletin
|December 9, 2025
概括
第一个持续活跃的快速无线电爆发 (FRB),FRB 20190520B,显示了快速分散度的下降. 这表明FRB位于一个密集的,不断膨胀的介质中,可能是超新星残留物.
科学领域:
- 天体物理学 天体物理学
- 无线电天文学 无线电天文学
背景情况:
- 快速无线电爆发 (FRB) 是神秘的,短暂的宇宙无线电短暂.
- 大多数FRB只被检测一次,这使得长期研究具有挑战性.
研究的目的:
- 为了识别和描述持久活跃的FRB源.
- 为了研究长期活跃FRB的分散度 (DM) 演变.
主要方法:
- 持续监测FRB来源的情况.
- 分散的分析测量随时间变化的变化.
主要成果:
- 确定FRB 20190520B作为第一个持续活跃的FRB超过4年.
- 在 (-12.4±0.3) pc cm-3yr-1的速度下,观察到DM的显著下降.
- 它的DM变化率是以前FRB的三倍,大小数级大于脉冲星.
结论:
- 观察到的DM进化和高宿主DM贡献表明FRB 20190520B处于密集,膨胀的电离介质中.
- 环境很可能是一个年轻的超新星残留物 (SNR).
关键词:
分散度指标是一种分散度指标.FRB 20190520B FRB 20190520B FRB 20190520B FRB 20190520B FRB 20190520B FRB 20190520B FRB 20190520B FRB 20190520B FRB 20190520B FRB 20190520B FRB 20190520B快速的无线电爆发就是快速的无线电爆发.传播效应是一种传播效应.这是一个超新星残余.更多相关视频
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