銀河とクエーザーの橋渡しをする 塵の多いコンパクトな物体
S Fujimoto1,2, G B Brammer3,4, D Watson3,4
1Cosmic Dawn Center (DAWN), Copenhagen, Denmark. fujimoto@nbi.ku.dk.
Nature
|April 14, 2022
まとめ
天文学者は初期の宇宙でユニークな物体である GNz7q を発見し,塵で覆われた星爆発段階の初期の超大質量ブラックホールを示し,クエーザーの進化の洞察を提供しました.
科学分野:
- 宇宙学と天体物理学
- 初期の宇宙のブラックホール形成
- 銀河の進化
背景:
- 初期の宇宙における 超大質量ブラックホールの形成は 重要な課題です
- ビッグバンから7億年後に 発光するクエサールが観測されました
- 模擬ではクエーザーは 塵で覆われた星爆発から 覆われない光の相へと進化します
研究 の 目的:
- 初期の宇宙における超大質量ブラックホールの形成と成長を調査する.
- 高赤偏移で変異するクエーザーを特定する.
- スターバースト銀河と 光るクエーサーの 進化のつながりを理解するために
主な方法:
- 紫外線コンパクト物体GNz7qの赤偏移7.1899の観測
- 深い高解像度画像と スリットレススペクトロスコーピー
- 塵の放射,星形成率,そしてX線の弱気分析.
主要な成果:
- GNz7qの発見 塵で覆われた星爆発銀河で 光る塵の放出がある
- GNz7q内の紫外線のコンパクトオブジェクトの識別
- GNz7qは非常に弱いX線放射を示し,新生ブラックホールまたはコンパクトな恒星形成領域を示唆しています.
結論:
- GNz7qは,未遮蔽の光るクエーザーの潜在的前身である.
- この発見はブラックホールとクエーザーの進化の宇宙学的シミュレーションと一致しています
- この発見は 超大質量ブラックホールの成長段階に関する 重要な観測証拠を提供します
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