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超大質量ブラックホールからのフィードバックによる初期型銀河の恒星形成の抑制
Kevin Schawinski1, Sadegh Khochfar, Sugata Kaviraj
1Department of Physics, University of Oxford, Oxford OX1 3RH, UK.
Nature
|August 25, 2006
まとめ
超大質量ブラックホールは,ガスを放出することで銀河の進化を調節し,巨大な銀河の恒星形成を抑制します. このフィードバックメカニズムは,銀河の恒星形成の歴史を理解するために非常に重要です.
科学分野:
- 天文学と天体物理学について
- 銀河の進化 銀河の進化 銀河の進化
- ブラックホール物理学 ブラックホール物理学
背景:
- 超大質量ブラックホールは銀河の中心部に存在し,フィードバックを通じてホスト銀河に影響を与えます.
- ブラックホールの性質と宿主銀河の特徴の間に観察された関係が存在する.
研究 の 目的:
- 超大質量ブラックホールのフィードバックが,大質量初期型銀河に与える役割を調査する.
- 恒星形成に影響を与える臨界ブラックホールの質量に対する経験的関係を導き出す.
主な方法:
- 巨大な初期型銀河からの紫外線放射の高解像度観測.
- ブラックホールの質量と宿主銀河の速度分散の分析.
主要な成果:
- 臨界ブラックホールの質量について,経験的関係が導き出された.
- この臨界質量以上のブラックホールからの流出は,冷たいガスを加熱して放出することで,星形成を抑制する.
結論:
- 超大質量ブラックホールは,質量が小さいにもかかわらず,銀河の恒星形成の歴史に重大な影響を及ぼします.
- ブラックホールのフィードバックは,巨大な銀河の恒星形成を調節する重要なメカニズムです.
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