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在形成大质量恒星的区域中,由磁场调节的自相似碎片化
Hua-bai Li1, Ka Ho Yuen1, Frank Otto1
1Department of Physics, The Chinese University of Hong Kong, Shatin, New Territory, Hong Kong, China.
Nature
|March 31, 2015
概括
磁场对于巨大的恒星形成至关重要. 在NGC 6334中,有序的磁场决定了气体在各种尺度上的碎片化,导致了延长的结构和异型收缩.
科学领域:
- 天体物理学 天体物理学
- 星星形成 星星形成
- 磁动力学是一种磁动力学.
背景情况:
- 分子云,通常是丝状的,形成恒星. 磁场影响低质量恒星的形成,形成云平行或垂直于云间场.
- 磁场在巨型恒星形成核心中的作用及其对中等尺度 (10到0.01帕塞克) 碎片化的影响仍然不清楚.
研究的目的:
- 研究磁场在巨型恒星形成区域的碎片化中的作用.
- 在NGC 6334中绘制磁场形态图,跨越广泛的尺度 (100到0.01帕塞克).
主要方法:
- 使用对NGC 6334的极度测量观测推断的磁场地图.
- 分析了场形态及其与多个尺度上的气体结构的关系.
主要成果:
- 在NGC 6334中观察到动态重要,有序的磁场,在不同尺度上一致.
- 发现了与自己相似的气体碎片,其长长的结构垂直于磁场.
- 在气体延长的末端发现密度峰值,对称地挤压场,场强度与密度^0.4成比例,表明异质收缩.
结论:
- 磁场在像NGC 6334.4这样的大型恒星形成区域内的气体碎片化中起着至关重要的作用.
- 观察到的异质气体收缩表明,磁场调节了大质量恒星形成中的积累过程.
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