Effects of Rotation and Thermohaline Mixing in Red Giant Stars

机译：红巨星自转和热盐混合的影响

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Thermohaline mixing has been recently identified as the probable dominating process that governs the photospheric composition of low-mass bright giant stars [Charbonnel and Zahn, A&A467, L15 (2007)]. Here we present the predictions of stellar models computed with the code STAREVOL including this mechanism together with rotational mixing. We compare our theoretical predictions with recent observations.

机译：近来，热盐混合被认为是控制低质量明亮巨星光球组成的可能主导过程[Charbonnel and Zahn，A＆A467，L15（2007）]。在这里，我们介绍了使用代码STAREVOL计算的恒星模型的预测，包括该机制以及旋转混合。我们将理论预测与最近的观察结果进行比较。

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《Red giants as probes of the structure and evolution of the Milky Way》|2012年|p.115-123|共9页
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Corinne Charbonnel; Nadege Lagarde; Patrick Eggenberger;
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Observatoire de Geneve, Universite de Geneve, 51 ch. des Maillettes 1290 Versoix, Switzerland Laboratoire d'Astrophysique de Toulouse-Tarbes, CNRS UMR 5572, Universite de Toulouse, 14 av. E.Belin 31400 Toulouse, France;

Observatoire de Geneve, Universite de Geneve, 51 ch. des Maillettes, 1290 Versoix, Switzerland;

Observatoire de Geneve, Universite de Geneve, 51 ch. des Maillettes, 1290 Versoix, Switzerland;

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正文语种 eng
中图分类恒星天文学、星系天文学、宇宙学;
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机译：热盐混合和低质量巨星的光球组成
2. Thermohaline mixing and the photospheric composition of low-mass giant stars [J] . F. C. Wachlin, M. M. Miller Bertolami, L. G. Althaus Astronomy and astrophysics . 2011,第19期

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机译：红巨星中旋转和温盐混合的影响

Effects of Rotation and Thermohaline Mixing in Red Giant Stars

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