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Updated: Jun 28, 2025

Setting Limits on Supersymmetry Using Simplified Models
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Published on: November 15, 2013

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恒星形成は,2.45の赤偏移で銀河の多相ガス流出によって停止した

Sirio Belli1, Minjung Park2, Rebecca L Davies3,4

  • 1Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy. sirio.belli@unibo.it.

Nature
|April 22, 2024
PubMed
まとめ

超大質量ブラックホールは 中性ガスを放出することで 巨大な銀河の恒星形成を迅速に止めることができます この研究は 遠くの銀河から 強力な中性ガス流出の 直接的な証拠を提供し 銀河の進化における その役割を確認しています

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