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Updated: Mar 20, 2026

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超大質量ブラックホールによる静止銀河の恒星形成抑制

Edmond Cheung1, Kevin Bundy1, Michele Cappellari2

  • 1Kavli Institute for the Physics and Mathematics of the Universe (World Premier International Research Center Initiative), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan.

Nature
|May 27, 2016
PubMed
まとめ

典型的な静止銀河では,低光度活性銀河核から中心に駆動された風が推論される. これらの風はガスを加熱し 星形成を抑制するのに十分なエネルギーを持ち 銀河の進化を説明します

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