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巨大な静止状態の II 群の銀河で赤道偏移は 2.1

Mariska Kriek1, Charlie Conroy2, Pieter G van Dokkum3

  • 1Department of Astronomy, University of California, Berkeley, California 94720, USA.

Nature
|December 9, 2016
PubMed
まとめ

巨大な円銀河は 宇宙の初期にほとんどの星を形成しました 赤い偏移 z=2.1 の銀河を研究したところ,高いマグネシウムと鉄の比率 ([Mg/Fe]) が明らかになり,早期の急速な星形成が示された.

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