銀河の進化 銀河の進化 銀河の進化 ブラックホールのフィードバックは,光るクワザール PDS 456 にある
E Nardini1, J N Reeves2, J Gofford2
1Astrophysics Group, School of Physical and Geographical Sciences, Keele University, Keele, Staffordshire ST5 5BG, UK. e.nardini@keele.ac.uk.
まとめ
クワザールPDS 456から離子化されたガスの持続的な相対論的流出が検出されました. この強力な風は,超大質量ブラックホールと銀河の共進化のメカニズムを示唆しています.
科学分野:
- 天体物理学 天体物理学
- 宇宙進化の宇宙進化について
- ブラックホール物理学 ブラックホール物理学
背景:
- 銀河の進化は,超大質量ブラックホール (SMBHs) の成長と密接に関連しています.
- クワザール相の間,SMBHは莫大なエネルギーを放出し,放射線駆動の風を通じて宿主銀河に影響を与えます.
研究 の 目的:
- SMBHと宿主銀河の共同進化を推進する物理的プロセスを調査する.
- 発光クワザールからの流出を検知し,特徴づけること.
主な方法:
- 五つの異なる時代における明るいクワザール PDS 456 のブロードバンドX線スペクトルの分析.
- 高イオン化ガスの流出を示すスペクトルシグネチャの識別.
主要な成果:
- 高度にイオン化されたガスの持続的,ほぼ球形の流出の検出.
- 流出は,相対的な速度で,蓄積円盤から放出されます.
- アウトフローの運動力は1秒あたり10~46 ergsを超え,重要なフィードバックポテンシャルを示している.
結論:
- 観測されたアウトフローは,クワザールにおける効果的なフィードバックメカニズムに対する強力な証拠を提供します.
- この発見は,SMBHと宿主銀河の共同進化のモデルを裏付けている.
- 流出の広い開口は,周囲の銀河環境との効率的な結合を示唆しています.
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