短命な分子雲と急速なフィードバックによる急速で非効率的な星形成
J M Diederik Kruijssen1,2, Andreas Schruba3, Mélanie Chevance4
1Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany. kruijssen@uni-heidelberg.de.
Nature
|May 24, 2019
まとめ
巨大な恒星は 恒星的なフィードバックによって ガス雲を素早く散らばらせて 恒星形成を短いサイクルに制限します これは 銀河の形成が予想より遅い理由を説明し 銀河の進化のダイナミックな構成要素を明らかにします
科学分野:
- 天文学と天体物理学
- 宇宙の進化
- 銀河の形成
背景:
- 星の形成と 星のフィードバックは 銀河の形成シミュレーションの 重要な不確実性です
- 巨大な分子雲の規模で これらのプロセスを理解することは 極めて重要です
- 星形成と雲のダイナミック・タイムスケールとの不一致は 未解明のままです
研究 の 目的:
- 巨大分子雲の分子ガスと 高質量恒星形成の関係を調査する
- 雲の進化と恒星形成の 規則を決定する
- 銀河の進化における 星のフィードバックの役割を理解するために
主な方法:
- スパイラル銀河NGC300の高角解像度観測
- 分子ガスと高質量星形成分布の分析
- 進化の時間軸を定量化するための統計的方法の適用
主要な成果:
- 分子ガスと高質量恒星形成は,巨大な分子雲のスケールで空間的に無関係です.
- このデコレーションは 雲,星形成,フィードバックの間の急速な進化サイクルを示しています
- 主に放射線と恒星風からの効率的なフィードバックは,約150万年以内に雲を分散させます.
結論:
- 雲の寿命は,恒星の急速なフィードバックによって,およそ1つのダイナミックな時間スケール (約1000万年) に制限されています.
- 雲の恒星形成の効率は低い (2〜3%).
- 銀河は 銀河の形成を形作る 活力のあるフィードバックによる ライフサイクルを 経由する 構成要素で構成されています
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