恒星HD14156969の周りを回る原惑星円盤のCOとH3と+である
Sean D Brittain1, Terrence W Rettig
1University of Notre Dame, Center for Astrophysics, Notre Dame, Indiana 46556, USA.
Nature
|July 5, 2002
まとめ
研究者らは,巨大な恒星HD141569.9の周辺で一酸化炭素 (CO) と水素 (H3+) の放出を検出した. この発見は,巨大な恒星の周りのガス巨大惑星の急速な形成に関する手がかりを提供します.
科学分野:
- 天文学と天体物理学について
- エクソプラネット科学 エクソプラネット科学
- 恒星とガスディスクのダイナミクス
背景:
- 数多くの恒星の周りに巨大な惑星が検出されていますが,ガス巨大惑星の形成の時間スケールは重要な問題です.
- 巨大な恒星は,周囲のガスを素早く分散させ,原惑星の核の増殖を阻害する可能性がある.
- Herbig AeBeの恒星 (2〜3倍の太陽の質量) の周りの原惑星を検出することは,惑星形成の時間スケールを制限することができます.
研究 の 目的:
- 巨大な恒星の周りの惑星形成のタイムスケールを調査するために.
- エルビグ・エーベの恒星HD141569.9の周りの原惑星円盤の進化の証拠を探すためでした.
- HD141569.9の円盤内のガスと潜在的な原惑星の分布を分析する.
主な方法:
- 原惑星円盤から排出される一酸化炭素 (CO) の検出.
- 原惑星円盤からの三水素カチオン (H3+) 放射の検出.
- ディスクの組成と構造を推論するために,排出データの解釈.
主要な成果:
- 5~10百万年前のハービグ・エービー星HD141569.9から検出されたCOとH3+の放射.
- COデータによると,内部円盤は17天文学単位以上,初期の蓄積段階を過ぎて,クリアされている.
- COとH3+の同時存在は驚くべきことであり,COは通常H3+を破壊する.
結論:
- 観測されたCOとH3+は円盤内で空間的に分離されている可能性があります.
- また,H3+の放出は,原惑星の大気圏から発生する可能性がある.
- この検出は,巨大な恒星の周りの惑星形成過程の重要な証拠を提供します.
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