一个年轻的双星原星中通过螺旋流和环恒星盘的气体流和积累
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.
概括
对年轻的双星原恒星系统[BHB2007]11的观测揭示了连接环恒星盘的复杂丝状结构. 收缩主要为质量较低的原恒星提供食物,与恒星多重性的理论模型保持一致.
科学领域:
- 天文学与天体物理学
- 恒星进化
- 恒星形成
背景情况:
- 大多数恒星存在于二进制或多进制系统中,影响它们的形成和进化.
- 研究年轻的双星原星提供了关于恒星多重性和轨道动态的关键数据.
研究的目的:
- 调查年轻的双星原恒星系统周围的环星盘的结构和动态 [BHB2007] 11.
- 在原蛋白环境中分析积累过程和外流现象.
主要方法:
- 进行了高角度分辨率的观测.
- 对圆盘形态和相关现象的详细分析.
主要成果:
- 原星系[BHB2007]11在每颗原星周围都有环恒星盘 (2-3 AU),其中包含几颗木星质量.
- 复杂的丝状结构将环恒盘与更大的环盘连接起来.
- 观测到积聚流和射电喷射,积聚有利于质量较低的原星.
结论:
- 观察到的积累模式支持二进制原星系统中质量转移的理论预测.
- 这些发现提供了对二进制恒星形成路径和早期演变的见解.
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