Studying p-mode damping and the surface effect with hydrodynamical simulations

被引：0

作者：

Kupka, F. ^{[1
]}

Belkacem, K. ^{[2
]}

Samadi, R. ^{[2
]}

Deheuvels, S. ^{[3
]}

机构：

[1] Univ Vienna, Fac Math, Wolfgang Pauli Inst, Oskar Morgenstern Pl 1, A-1090 Vienna, Austria

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

[3] Univ Toulouse, UPS OMP, IRAP, F-31400 Toulouse, France

来源：

SECOND BRITE-CONSTELLATION SCIENCE CONFERENCE - SMALL SATELLITES - BIG SCIENCE | 2017年 / 5卷

基金：

奥地利科学基金会;

关键词：

CONVECTION; COROT; OSCILLATIONS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Hydrodynamical simulations can be used as a complementary tool to observations for the study of the damping of p-modes and the so-called surface effect in solar-like oscillators. Here, we present the state-of-the-art in this research. Examples of applications include our Sun and the CoRoT target stars HD 49385 and HD 49933.

引用

页码：222 / 227

页数：6

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