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红色超巨星安塔雷斯的强烈大气运动
K Ohnaka1, G Weigelt2, K-H Hofmann2
1Instituto de Astronomía, Universidad Católica del Norte, Avenida Angamos 0610, Antofagasta, Chile.
Nature
|August 18, 2017
概括
研究人员绘制了红色超巨星安塔雷斯的速度场, 在大气层中发生的这些动荡运动表明,
科学领域:
- 恒星天体物理学
- 天文学
- 大气动力学
背景情况:
- 红色超巨星是有复杂大气层的巨星.
- 之前的研究使用光谱来探测红色超巨星的大气层.
- 在这些大气层中发现了亮点.
研究的目的:
- 为了绘制红超巨星安塔雷斯的二维速度场.
- 调查其扩展大气层的动态.
- 识别导致大气运动的过程.
主要方法:
- 近红外光谱干扰成像
- 在恒星的表面和大气中绘制气体速度.
- 分析恒星大气动力学.
主要成果:
- 观察到气体团的强烈上升和下降运动.
- 速度在-20到+20公里/秒之间.
- 大气层延伸到大约1.7星半径.
结论:
- 观察到的流运动超出了单靠对流的解释.
- 一个未知的过程可能驱动扩展大气中的动力.
- 需要进一步的研究来理解这一现象.
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