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z = 2.626 の銀河の元素の豊富なパターン

Jason X Prochaska1, J Christopher Howk, Arthur M Wolfe

  • 1UCO/Lick Observatory, University of California, Santa Cruz, California 95064, USA. xavier@ucolick.org

Nature
|May 2, 2003
PubMed
まとめ

天文学者は,遠い銀河の25以上の元素を測定し,その化学的濃縮の歴史を明らかにしました. 発見は,巨大な恒星が主要な源であることを示唆し,銀河の進化と核合成の洞察を提供している.

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