青い恒星形成銀河における9〜11の赤道移転で強い緩んだライマンα吸収

Kasper E Heintz1,2, Darach Watson1,2, Gabriel Brammer1,2

  • 1Cosmic Dawn Center, Copenhagen, Denmark.

Science (New York, N.Y.)
|May 23, 2024
PubMed
まとめ

初期の銀河には 驚くほど大量の中性原子水素 (H I) が含まれており 恒星形成に不可欠です JWSTを用いたこの発見は 初期の宇宙と銀河の進化に関する以前のモデルに 異議を唱えます

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