ブラックホールの活動によって調節されるアニゾトロプ衛星銀河の消火
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PubMedで要約を見る
まとめ
この要約は機械生成です。超大質量ブラックホールは物質を放出することで 衛星銀河の進化に影響を与えます この流れは,特に小軸に沿って,衛星銀河の星形成を保ちます.
科学分野
- 天体物理学
- 銀河の進化
- 宇宙学
背景
- 衛星銀河の進化は,環銀河媒介との相互作用によって影響を受けます.
- 中央の超大質量ブラックホールの活動がこの媒介に与える影響は,限られた観測証拠で議論されている.
研究 の 目的
- 超大質量ブラックホールのフィードバックと 衛星銀河の進化の関係を調べるため
- 中心銀河に比べて 消えた衛星銀河の空間分布を分析する.
主な方法
- ダークマターハロー内の 124,163 衛星銀河のアーカイブデータの分析.
- 観測データとIllustrisTNG宇宙シミュレーションの結果を比較する.
主要な成果
- 消えた衛星銀河は 中央銀河の小軸に沿って 少なく見られます
- このアニゾトロプ的分布は,環銀河媒体をクリアする活性銀河核 (AGN) の流出に起因する.
結論
- 超大質量ブラックホールのフィードバックは 衛星銀河の進化を形作る上で 重要な役割を果たします
- アウトフローはラームの圧力を減らし,衛星銀河の恒星形成をシミュレーションで同位反射モデルでも保存します.
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