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銀河系 の 核 風 に 含ま れ て いる 冷たい ガス
Enrico M Di Teodoro1,2,3, N M McClure-Griffiths4, Felix J Lockman5
1Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA. editeodoro@jhu.edu.
Nature
|August 21, 2020
まとめ
科学 者 たち は 銀河 から 流れる 寒い 密集 し た 分子 ガス を 発見 し まし た
科学分野:
- 天体物理学
- 銀河の力学
- 星間メディア
背景:
- 銀河の中心は 射手座A*からの高エネルギープロセスと 星のフィードバックを経験しています
- 銀河の円盤から物質とエネルギーを 放出します
- 観測された流出ガスは,熱いイオン化,暖かいイオン化,冷たい原子相を含む.
研究 の 目的:
- ミルクウェイの銀河風の中の 寒くて密度の高い分子ガスの存在と性質を 調べるために
- 以前は観測されていなかった ガス相の起源と影響を理解するために
主な方法:
- 高解像度で分子ガスの流出を観測した.
- 寒いガス雲の形態と運動の分析
- 核風の中の原子水素雲との関連
主要な成果:
- 銀河の中心から冷たく密集した分子ガスを 直接観測した.
- 分子ガスの雲は 熱い流出媒介と混じり合って 破壊される可能性があります
- 分子流出の質量は重要で,中央の星形成に影響を与える可能性があります.
結論:
- 銀河の風の中の冷たい分子ガスの発見は 既存のモデルに挑戦しています
- 現在の Sagittarius A*の活動も中央の星形成も,このガスの存在を完全に説明できません.
- この冷たいガスが 銀河の進化や星形成に 重要な役割を果たすかもしれません
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