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Updated: Feb 15, 2026

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[C ii]を放出するガスの回転は,6.8の赤偏移で2つの銀河で

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
まとめ

研究者らは,2つの初期の銀河からの炭素2 ([C ii]) 放射線を検出し,再イオン化の時代に関する新しい洞察を提供しました. これらの発見は,驚くほど明るい [C ii]信号を明らかにし,初期の銀河のダイナミクスは,宇宙の歴史においてずっと後に見られたものと同じであることを示唆しています.

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