在13颗类似太阳的恒星中探测度旋转差异
O Benomar1, M Bazot2, M B Nielsen2
1Center for Space Science, New York University, Abu Dhabi (NYUAD), UAE. othman.benomar@nyu.edu.
概括
研究人员使用星体地震学测量了恒星的旋转, 发现赤道速度比预测更快. 在类似太阳的恒星中,
科学领域:
- 恒星天体物理学
- 天体地震学和星体地震学
背景情况:
- 恒星外层的旋转差对于磁性活动至关重要.
- 产生和维持差分旋转的机制仍然不太清楚.
研究的目的:
- 测量类似太阳恒星的对流区域的度差旋转.
- 将星际地震测量与理论预测进行比较.
主要方法:
- 使用星体地震学探测恒星的内部结构和旋转.
- 分析了40颗类似太阳的恒星的数据,
主要成果:
- 成功测量了40颗类似太阳的恒星的对流带的度分旋.
- 在重要的检测中观察到的赤道旋转速度大约是中度速度的两倍.
- 推断的度剪切明显超过当前数值模拟的预测.
结论:
- 星体地震学为测量恒星的不同旋转提供了强大的工具.
- 目前的模型可能低估了恒星对流区的度切割程度.
- 观测到的大度剪切对恒星动力学理论和磁性活动有影响.
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