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Updated: Mar 25, 2026

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快速无线电爆发的宿主星系
E F Keane1,2,3, S Johnston4, S Bhandari2,3
1Square Kilometre Array Organisation, Jodrell Bank Observatory, SK11 9DL, UK.
快速无线电爆发 (FRB) 是一种神秘的宇宙信号. 这项研究将FRB与宿主星系联系起来,测量其红移,并提供关于星系间介质和缺失的子的关键数据.
科学领域:
- 宇宙学
- 天体物理学
- 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.
- 散射测量是FRB的关键可观测量, 但红移测量一直是具有挑战性的.
- 之前的FRB研究缺乏宿主星系的识别和红移数据.
研究的目的:
- 报告发现了一种具有精确测量红移的快速无线电爆发.
- 使用分散度和红移来限制离子化子的宇宙密度.
- 为了研究原始模型和快速无线电爆发的性质.
主要方法:
- 检测快速无线电爆发 (FRB).
- 在FRB之后识别了~6天的色无线电瞬态.
- 主星系的识别及其红移的测量 (z = 0.492 ± 0.008).
主要成果:
- 在星系间介质中直接测量离子化子的宇宙密度 (ΩIGM = 4.9 ± 1.3%).
- 测量到的 ΩIGM 与威尔金森微波异型探测器 (WMAP) 的预测一致,并解释了所有"缺失的子".
- ~6天的无线电短暂与短暂的马射线爆发相一致,表明至少有两种类型的FRB.
结论:
- 这项研究首次使用FRB直接测量了星系间介质的离子密度.
- 这些发现支持宇宙网络中大量的电离子存在.
- 这些结果挑战了一些FRB的原始模型,并表明它们的起源多样化.
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