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ミルクウェイのペルセウスの腕にある銀河の煙突
M Normandeau1, A R Taylor, P E Dewdney
1Department of Physics and Astronomy, University of Calgary, Alberta, Canada.
Nature
|April 25, 1996
まとめ
熱いガスの輸送のための管である銀河の煙突は,ペルセウスの腕にある新しい原子水素の地図によって証明されています. 巨大な恒星風によって形成された可能性が高いこれらの構造は,銀河の円盤をハロに結びつける.
科学分野:
- 天体物理学 天体物理学
- 銀河系天文学 銀河系天文学
- 星間媒介は,星間媒介である.
背景:
- 銀河には熱いガスのハロがあり,そのガスが冷却するにつれて補充する必要があります.
- 銀河の"煙突"は,星間媒体の理論上の空洞であり,超新星爆発によって形成された可能性がある.
- これらの煙突は,銀河円盤からホットガスのハロへの輸送を容易にすると仮定されています.
研究 の 目的:
- 高解像度の原子水素マッピングデータを提示するために.
- 銀河の煙突の存在に対する観察的証拠を提供するため.
- 銀河の煙突の形成と現在の状態を調査する.
主な方法:
- 原子水素の高解像度マッピング.
- 私たちの銀河のペルセウスの腕の分析.
主要な成果:
- 銀河の煙突の存在の明確な証拠は,ペルセウスの腕で見つかりました.
- 煙突は,若い,巨大な星群からのエネルギーに満ちた風によって形成されたようです.
- 煙突は,銀河のハローに広がる段階に達しているかもしれません.
結論:
- 観測の証拠は,銀河の煙突の概念を支持しています.
- 巨大な恒星風は,煙突形成の合理的なメカニズムである.
- 銀河の煙突は,銀河の円盤とハロの間のガスのダイナミックな交換に役割を果たします.
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