气体通过一个原行星间隙流动
Simon Casassus1, Gerrit van der Plas, M Sebastian Perez
1Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile. scasassus@u.uchile.cl
Nature
|January 4, 2013
概括
观测显示,气体通过年轻恒星HD 142527的原行星盘的空隙流动,表明行星形成正在积极地滋养恒星积聚. 这种气体流对于维持恒星至关重要.
科学领域:
- 天文学和天体物理学
- 行星科学 行星科学
背景情况:
- 行星形成模型预测原行星盘中的空隙.
- 年轻的恒星HD 142527表现出一个内部圆盘,一个大的空隙,和一个被破坏的外部圆盘.
研究的目的:
- 为了研究HD 142527原行星盘的隙间内的气体动态.
- 为了确定气体流能否维持观测到的高恒星积聚率.
主要方法:
- 红外观测绘制磁盘结构的地图.
- 无线电观测用于分析分子气体的组成和分布.
- 在隙中分析分散的CO和密集的HCO+气体.
主要成果:
- 在隙内检测到分散的CO气体.
- 沿着穿过隙的细丝观察到更密集的HCO+气体.
- 估计气体流速为每年7x10^-9至2x10^-7太阳质量.
结论:
- 观察到的气体流量足以维持恒星的高积累率.
- 原行星体可能会将气体从外盘转向内盘.
- 这为正在进行的行星形成提供了证据,影响着恒星活动.
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