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サブミリメートルの波長で明るく輝く銀河の赤道偏移の平均値は2.4です

S C Chapman1, A W Blain, R J Ivison

  • 1California Institute of Technology, Pasadena, California 91125, USA.

Nature
|April 18, 2003
PubMed
まとめ

塵に隠された初期の宇宙の銀河は,サブミリメートル (submm) の観測を通して明らかになる. スペクトル学的な赤偏移は,これらの輝く塵の星系がクエザールと共存し,宇宙の進化に影響を与えたことを示しています.

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