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遠赤外線背景光の半分以上は,z >or= 1.2の銀河から来ている

Mark J Devlin1, Peter A R Ade, Itziar Aretxaga

  • 1Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, Pennsylvania 19104, USA. devlin@physics.upenn.edu

Nature
|April 11, 2009
PubMed
まとめ

サブミリメートルの調査では,遠赤外線背景光 (FIRB) のほとんどは,高赤偏移の明るい銀河から発生していることを明らかにしています. z > 1.2で観測されたこれらの塵の星爆発銀河は,この宇宙放射線の主な貢献者です.

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