Lithium Depletions in Late-type Dwarfs
Using a self-consistant dynamic theory of non-local convection in chemically inhomogeneous stars,the lithium depletion in MS stars of masses 0.725 1.5 M are calculated. Both of the overshooting and microdiffusion are included in a consistent way. The comparisons of theretical reasults with the observed Li depletions in open clusters show that the general characters of Li depletions can be reproduced by theory. The overshooting mixing and microdiffusion induced by gravitational setting and radiative accelerations may be two main mechanisms of Li depletion.
Convection- star abundance-star late-type-stars evolution- open clusters and associations general
D.R.Xiong L.Deng
Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008 National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012
国际会议
The 252th Symposium of the International Astronomical Union(国际天文学联合会第252届研讨会)
海南三亚
英文
61-66
2008-04-06(万方平台首次上网日期,不代表论文的发表时间)