IRC+10216の周りの水蒸気の発見は,他の恒星の周りを回っている彗星の証拠として使用されました
G J Melnick1, D A Neufeld, K E Saavik Ford
1Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA. gmelnick@cfa.harvard.edu
Nature
|July 13, 2001
まとめ
天文学者は,炭素星IRC+10216の周りに水蒸気を検出しました. これは,近年の恒星の明るさの増加により,軌道上の氷の体が蒸発してい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
- 惑星外科学とは,惑星外科学です.
背景:
- 1995年以来,スペクトルシフトから推論された恒星の反射運動によって,木星の質量の系外惑星が検出されています.
- この半径速度法では,太陽系に似た小さな天体を検出するには不十分です.
研究 の 目的:
- 進化した炭素星IRC+10216.6の周りの環恒星物質の組成を調査する.
- 小さい軌道上の天体を検出するための代替方法を探求する.
主な方法:
- スペクトル解析を用いた周周水蒸気の観測.
- 進化した炭素星IRC+10216の輝度変化の分析.
主要な成果:
- IRC+10216.6の星周環境で有意な水蒸気の検出
- 水蒸気は炭素星の周りに測定可能な量では通常予想されません.
結論:
- 観測された水蒸気は,軌道上の氷の体の蒸発を強く示唆しています.
- この現象は,IRC+10216の明るさが最近大幅に増加したことと関連しています.
- この発見は,進化する恒星の周りの氷の体蒸発の理論的モデルを裏付けている.
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