Overshooting in stars: Five old fallacies and a new model

被引：30

作者：

Canuto, VM

机构：

[1] NASA, Goddard Institute for Space Studies, New York, NY 10025

来源：

ASTROPHYSICAL JOURNAL | 1997年 / 489卷 / 01期

关键词：

convection; stars; kinematics; turbulence;

D O I：

10.1086/310955

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

First, I discuss five fallacies of previous theoretical attempts to quantify overshooting in stars. I then suggest that the only reliable procedure is to solve the five dynamic equations for convective flux, kinetic and potential energy, turbulent pressure and dissipation rate of kinetic energy, plus the mean temperature equation. Finally, I discuss a recent solution of the new model that agrees with the latest helioseismological OV data and suggest that the same data be used to check the validity of the Schwarzschild criterion.

引用

页码：L71 / L74

页数：4

共 22 条

[1] NEW STRONG EVIDENCE FOR THE IMPORTANCE OF CONVECTIVE OVERSHOOTING IN INTERMEDIATE-MASS STARS [J].