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Controlling Flow Speeds of Microtubule-Based 3D Active Fluids Using Temperature
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ブラックホールの蓄積円盤からの風は,活発な銀河の分子流出を駆動する

F Tombesi1, M Meléndez2, S Veilleux3

  • 11] X-ray Astrophysics Laboratory, NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA [2] Department of Astronomy and CRESST, University of Maryland, College Park, Maryland 20742, USA.

Nature
|March 27, 2015
PubMed
まとめ

科学者たちは,超明るく輝く銀河で強力な蓄積円盤風を検知し,クエーザーのフィードバックメカニズムを確認した. この発見は,超大質量ブラックホールの活動と銀河の進化を結びつけ,風が恒星形成を抑制する方法を説明します.

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