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GRB 090423はzの赤偏差で約8.1であった

R Salvaterra1, M Della Valle, S Campana

  • 1INAF, Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807 Merate (LC), Italy. salvaterra@mib.infn.it

Nature
|October 30, 2009
PubMed
まとめ

天文学者は,z = 8.1.1.の記録的な赤偏移でガンマ線爆発 (GRB) を検出した. この初期の宇宙のGRBは,ビッグバン直後に同様の恒星爆発メカニズムが存在していたことを示唆しています.

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