在棕矮星盘中行星形成的开始
Dániel Apai1, Ilaria Pascucci, Jeroen Bouwman
1Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA. apai@as.arizona.edu
概括
行星形成过程,包括尘埃的生长和沉,发生在棕矮星周围的冷盘中,类似于恒星周围的冷盘. 这表明行星形成是年轻环恒星盘中常见的过程.
科学领域:
- 天文学和天体物理学
- 外系行星科学 外系行星科学
背景情况:
- 星球的形成始于尘埃粒的生长和沉积在原行星盘中.
- 这些过程在低质量和中质量恒星周围的磁盘中得到了充分研究.
研究的目的:
- 为了研究棕矮星周围盘中的行星形成过程.
- 为了比较棕矮星盘中的尘埃演变与恒星盘.
主要方法:
- 从棕矮星和候选星体周围的磁盘中获取和分析红外光谱.
- 观察到的光谱特征与尘埃生长和沉积模型的比较.
主要成果:
- 红外光谱揭示了灰尘的生长和沉积在棕矮星周围的磁盘中.
- 这些过程与围绕恒星的圆盘中观察到的类似或相同.
结论:
- 行星形成的开始发生在棕矮星周围的冷盘中.
- 行星形成是一个强大的过程,在大多数年轻的环恒星盘中很可能是常见的,无论中心物体的质量如何.
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