相关实验视频
Updated: May 10, 2026

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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
一个群体的快速无线电爆发在宇宙学距离
D Thornton1, B Stappers, M Bailes
1Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester, UK. thornton@jb.man.ac.uk
概括
天文学家发现了四个来自遥远星系的快速无线电爆发 (FRB). 这些宇宙信号可以帮助科学家测量宇宙的物质含量.
科学领域:
- 天体物理学 天体物理学
- 宇宙学的宇宙学是什么?
- 无线电天文学 无线电天文学
背景情况:
- 暂时的天体物理来源为物理过程提供了独特的见解.
- 对脉冲星和快速过渡体的调查是发现新型天体的关键.
研究的目的:
- 报告发现了四个毫秒持续时间的无线电瞬态.
- 描述这些短暂的物质,并探索它们作为宇宙学探测器的潜力.
主要方法:
- 使用对脉冲星和快速过渡体的调查.
- 分析爆发特性以确定天文起源.
- 使用宿主星系和星系间介质模型来估计红移和距离.
主要成果:
- 检测到四个持续数毫秒的无线电瞬态,距离银河系平面超过40°.
- 爆发特性证实了它们的天文起源.
- 估计的宇宙红移在0.5到1之间,距离高达3千兆秒.
- 没有观察到相关的X射线或玛射线标志.
结论:
- 这些无线电短暂物体代表了一类新的银河系外短暂源.
- 它们的宇宙学距离使得它们对于探测星际介质非常有价值.
- 描述源群和宿主星系的特征,可以帮助确定宇宙的重子含量.
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