一个年轻的原行星盘中的螺旋密度波
Laura M Pérez1, John M Carpenter2, Sean M Andrews3
1Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany. lperez@mpifr-bonn.mpg.de.
概括
天文学家使用阿塔卡马大毫米/亚毫米阵列探测到一颗年轻恒星原行星盘的中平面. 这些结构可能表明盘子中最密集区域的行星形成活动.
科学领域:
- 天文学
- 天体物理学
- 星球科学
背景情况:
- 理论上,螺旋密度波是由于引力而形成的.
- 之前对原行星盘中的螺旋结构的观测无法探测中间平面,其中大部分磁盘质量存在,行星形成发生.
研究的目的:
- 在原行星盘的中平面研究螺旋密度波.
- 确定是否可以观察到螺旋结构到达磁盘中平面.
主要方法:
- 使用阿塔卡马大毫米/亚毫米阵列 (ALMA) 进行高分辨率观测.
- 分析了来自年轻恒星Elias 2-27的原行星盘的毫米波辐射.
主要成果:
- 在伊利亚斯2-27原行星盘中检测到一对相对应的螺旋臂.
- 证实这些螺旋臂延伸到磁盘的外部区域, 并可追溯到中间平面.
- 观察到螺旋臂内部的发射间隙,靠近中心恒星.
结论:
- 探测到的螺旋臂可能代表密度波在磁盘中平面传播的冲击.
- 这些发现为原行星盘的行星形成区域中发生的现象提供了观察证据.
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