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Updated: Feb 15, 2026

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在两个星系的[C ii]发射气体中以6.8的红移旋转

Renske Smit1,2, Rychard J Bouwens3, Stefano Carniani1,2

  • 1Cavendish Laboratory, University of Cambridge, 19 JJ Thomson Avenue, Cambridge CB3 0HE, UK.

Nature
|January 12, 2018
PubMed
概括

研究人员发现了两个早期星系的二氧化碳 ([C ii]) 排放线,为再电离时代提供了新的见解. 这些发现揭示了令人惊的[C ii]信号,

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