EXCITATION OF INTERNAL GRAVITY WAVES BY PENETRATIVE CONVECTION

被引：0

作者：

Pincon, C. ^{[1
]}

Belkacem, K. ^{[1
]}

Goupil, M. J. ^{[1
]}

机构：

[1] Univ Paris Diderot, PSL Res Univ, Univ Pierre & Marie Curie, CNRS,LESIA,Observ Paris, F-92195 Meudon, France

来源：

ASTRO FLUID 2016 | 2019年 / 82卷

关键词：

D O I：

10.1051/eas/1982024

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We investigate the ability of internal gravity waves that are generated by penetrative convection to redistribute angular momentum in the internal radiative zone of evolved low-mass stars. To do so, we use the semianalytical excitation model recently proposed by Pinson et al. 2016. We briefly report the preliminary results of the study focusing on the subgiant and red giant branch stars.

引用

页码：247 / 251

页数：5

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