Chris A Collins1, John P Stott, Matt Hilton

  • 1Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead, CH41 1LD, UK. cac@astro.livjm.ac.uk

Nature
|April 3, 2009
PubMed
まとめ

最も明るい銀河団は,ビッグバンからわずか45億~50億年後に,その恒星質量の90%以上をほぼ完全に構成していた. この発見は銀河形成モデルに異議を唱え,長期にわたる階層的構成ではなく,急速な初期の成長を示唆しています.

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