5.7C IV[C II]

Daichi Kashino1,2, Simon J Lilly3, Robert A Simcoe4

  • 1Institute for Advanced Research, Nagoya University, Nagoya, Japan. kashinod.astro@gmail.com.

Nature
|May 10, 2023
PubMed
概括

我们检测到两个[C sup II]发射星系在红移5.7附近, 与高离子化气体系统相关. 这些星系表现出紧的尺寸和狭窄的线宽,这表明在宇宙再离子化过程中出现了模糊的恒星形成.

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