在红移2.6的星系中,来自尘埃的极化热辐射
J E Geach1, E Lopez-Rodriguez2, M J Doherty3
1Centre for Astrophysics Research, School of Physics, Engineering and Computer Science, University of Hertfordshire, Hatfield, UK. j.geach@herts.ac.uk.
Nature
|September 6, 2023
概括
早期的星系迅速形成了有序的磁场, 这对于恒星形成至关重要. 观测揭示了遥远星系中的5千帕斯克级磁场,显示这些结构在宇宙历史中迅速发展.
科学领域:
- 天体物理学
- 宇宙进化
- 银河系动力学
背景情况:
- 磁场对于星系进化,星际介质和恒星形成至关重要.
- 大规模的磁场已知在附近的星系, 但他们的早期宇宙的形成是不清楚的.
研究的目的:
- 在早期宇宙中研究磁场的形成和结构.
- 为了确定星系中有序磁场是否迅速形成.
主要方法:
- 来自尘埃粒的线性极化热辐射的检测.
- 一个强烈的透镜,发光的星系在红移2.6的观测.
- 对尘埃粒与当地的磁场对齐的分析.
主要成果:
- 检测到一个5千帕秒级的磁场.
- 估计磁场强度大约为500μG或更低.
- 极化分数约为1%,类似于附近的螺旋星系.
- 磁场与分子气体盘平行.
结论:
- 在星系中可以快速形成有序的磁场.
- 这些结构存在于宇宙历史的早期.
- 这些发现支持磁场在早期星系进化和恒星形成中的作用.
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