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Assembly of Complex Microtubule Structures
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非常年轻的原恒星星团Serpens South中的偶发性分子外流
Adele L Plunkett1, Héctor G Arce1, Diego Mardones2
1Astronomy Department, Yale University, New Haven, Connecticut 06511, USA.
Nature
|November 6, 2015
概括
原恒星的外流表现出偶尔发生的质量喷射事件,即使是在密集星团中恒星形成的最早阶段. 这为这些环境中的恒星形成提供了关键的动荡.
科学领域:
- * 天文学与天体物理学
- * 恒星的形成和演变
- * 原星体喷流和外流
背景情况:
- *原星质量积累伴随着通过喷气或外流的质量损失.
- * 在0类和I类原恒星阶段观察到偶发的喷射事件.
- * 在密集的恒星形成星团中,外流的行为尚不清楚.
研究的目的:
- * 在聚星环境中研究年轻原星的积聚驱动的外流的性质.
- * 为了确定星团内部的原恒星进化的早期阶段是否发生了偶发的喷射事件.
- * 了解前恒星团中外流在转移动量和能量中的作用.
主要方法:
- * 在南蛇星团的中心观测一个年轻的0类原星.
- 分析 (12) C(16) O (J=2-1) 排放以确定外流喷射特征.
- * 检查C(18) O外排放以研究内落和旋转动力学.
主要成果:
- * 发现了来自原恒星的偶发性外流喷射事件的明确证据.
- * 检测到22个不同的外流喷射特征,最近显示的速度最高.
- * 外流形成从1毫米连续发射峰开始的双极叶,周围的外显示内落和旋转.
结论:
- * 偶发的,由积累驱动的外流开始于前恒星进化的早期阶段.
- *原恒星的外流可以保持完整,并在密集的集群环境中运行.
- 这些外流可能通过集群中的高效动量转移在驱动流中发挥重要作用.
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