论文标题
来自太阳能和恒星地震学的低质量恒星的内部旋转
The internal rotation of low-mass stars from solar and stellar seismology
论文作者
论文摘要
通过螺旋志和星星志学测量太阳和恒星的内部旋转的可能性为作用于恒星内部的水力和磁流失动力学过程提供了巨大限制。了解负责在恒星内部中角动量运输的过程至关重要，因为它们还将影响化学物质的运输，从而影响恒星的演变。在这里，我们介绍了两个领域中获得的一些关键结果，以及如何对低质量恒星内部角动量传输物理的详细地震分析提供严格的约束，并有可能排除某些候选者。
The possibility of measuring the internal rotation of the Sun and stars thanks to helio- and asteroseismology offers tremendous constraints on hydro- and magnetohydrodynamical processes acting in stellar interiors. Understanding the processes responsible for the transport of angular momentum in stellar interiors is crucial as they will also influence the transport of chemicals and thus the evolution of stars. Here we present some of the key results obtained in both fields and how detailed seismic analyses can provide stringent constraints on the physics of angular momentum transport in the interior of low mass stars and potentially rule out some candidates.
