茶色矮星から物質の流れが解消された
Emma T Whelan1, Thomas P Ray, Francesca Bacciotti
1Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland. ewhelan@cp.dias.ie
Nature
|June 3, 2005
まとめ
生まれたばかりの茶色矮星,または"失敗した星"は,若い星と似ていますが,より小さなスケールで超音速の流出を示します. この発見は,物質の放出が恒星と惑星の形成における普遍的なメカニズムであることを示唆しています.
科学分野:
- 天文学と天体物理学について
- 星の形成と進化について
背景:
- 星の誕生には,超音速の流出経由で物質の蓄積と排出の両方が含まれます.
- この流出現象は,若い恒星ではよく記録されています.
- 星と惑星の間の"失敗した星"である茶色矮星でも同様の流出が発生するかどうかは不明です.
研究 の 目的:
- 新生茶色矮星が超音速外流を発揮するかどうかを調査するために.
- 茶色矮星からの流出を空間的に解明し,特徴づけるために.
主な方法:
- 流出する物質を空間的に解明するために,スペクトロアストロメトリックデータを利用しました.
- 観測されたブラウン・ダワーフ・アウトフローの特徴を分析した.
主要な成果:
- ブラウン・ダワーから発生した超音速流出が解決され,確認されました.
- 流出の特徴は,若い星の特徴に匹敵するが,それより縮小されている.
結論:
- アウトフローを駆動するメカニズムは,星や茶色矮星全体に共通しているようです.
- この普遍的な流出メカニズムは,惑星の形成に役割を果たす可能性がある.
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