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Updated: May 20, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
一个前棕矮星的干涉测量识别.
Philippe André1, Derek Ward-Thompson, Jane Greaves
1Laboratoire d'Astrophysique, Instrumentation et Modélisation (AIM), Commissariat à l'Energie Atomique (CEA)/Direction des Sciences de la Matière (DSM)-CNRS-Université Paris Diderot, Gif-sur-Yvette, France. philippe.andre@cea.fr
概括
研究人员确定了棕矮星前的核心,支持棕矮星像恒星一样形成的理论. 这种气体和尘埃凝聚的质量在棕矮星范围内.
科学领域:
- 天文学和天体物理学
- 星星形成的形成
- 棕矮人的研究研究
背景情况:
- 棕矮星的形成机制,这些物体的质量低于燃烧极限 (0.075太阳质量),仍然不确定.
- 人们还在争论棕矮星是以类似于太阳类型恒星的方式形成的还是通过其他过程形成的.
研究的目的:
- 为了研究棕矮星的形成过程.
- 提供支持或反对现有的棕矮星形成模型的观测证据.
主要方法:
- 利用毫米干扰度观测来检测热连续辐射.
- 分析了辐射,以确定物体的质量和半径.
- 测量了光谱线宽度以推断动态质量.
主要成果:
- 成功地确定了棕矮星质量体制中的自我引力气体和尘埃凝聚.
- 该物体的热辐射表明其质量约为0.02到0.03太阳质量.
- 一个小的半径 (<460天文单位) 和狭窄的光谱线表明一个动态质量在0.015和0.02太阳质量之间.
结论:
- 这种棕矮星前核心的发现为棕矮星通过与燃烧恒星相同的过程形成的模型提供了强有力的支持.
- 这一发现有助于统一对恒星和棕矮星形成途径的理解.
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