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Updated: Apr 7, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
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銀河系の進化. ビッグバンから20億年後の典型的な恒星形成銀河の超大質量ブラックホールです

Benny Trakhtenbrot1, C Megan Urry2, Francesca Civano3

  • 1Department of Physics, Institute for Astronomy, ETH Zurich, Wolfgang-Pauli-Strasse 27, Zurich 8093, Switzerland. benny.trakhtenbrot@phys.ethz.ch.

Science (New York, N.Y.)
|July 11, 2015
PubMed
まとめ

初期の宇宙時代は,超大質量ブラックホール (SMBH) が宿主銀河よりも効率的に成長することを示し,共進化モデルに挑戦しています. 激しい恒星形成は,SMBHによる流出にもかかわらず継続しています.

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