若い双星原星における螺旋流と環状円盤によるガス流と蓄積
F O Alves1, P Caselli2, J M Girart3,4
1Center for Astrochemical Studies, Max Planck Institute for Extraterrestrial Physics, Garching, 85748, Germany. falves@mpe.mpg.de.
まとめ
若いバイナリー原星系 [BHB2007] 11の観測により,周周円盤を結ぶ複雑な線状構造が明らかになった. 収縮は優先的に低質量プロトスターに供給し 恒星の多重性の理論モデルと一致します
科学分野:
- 天文学と天体物理学
- スター進化
- 星の形成
背景:
- ほとんどの恒星は2つ星系または複数の星系で存在し,その形成と進化に影響を与えています.
- 若きバイナリー原星を研究することで 恒星の多様性や軌道動態に関する重要なデータが得られます
研究 の 目的:
- 若き二重原星系の周りの円盤の構造と動態を調査する [BHB2007] 11.
- プロトバイナリ環境における蓄積過程と流出現象を分析する.
主な方法:
- 高角解像度観測が行われました.
- 円盤形状と関連する現象の詳細な分析
主要な成果:
- 原星系[BHB2007]11は,いくつかの木星質量を含む各原星周りの周回円盤 (2-3AU) を特徴としています.
- 複雑な繊維構造は,周周円盤とより大きな周周周円盤を結びつける.
- 蓄積流とラジオジェットが観測され,蓄積は低質量プロトスターを好む.
結論:
- 観測された蓄積パターンは,二重星系における質量移転の理論的予測を支持する.
- この発見は 二重星の形成経路と初期進化の洞察を与えてくれます
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