Sodium excess in yellow supergiants: Implications for rotational mixing in massive main-sequence stars

被引:10
作者
Denissenkov, PA [1 ]
机构
[1] Univ Victoria, Dept Phys & Astron, Victoria, BC V8W 3P6, Canada
关键词
stars : abundances; stars : evolution; stars : interiors; stars : rotation;
D O I
10.1086/428393
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent high-quality measurements of the sodium abundance in yellow supergiants are used to test the hypothesis of rotational mixing in massive main-sequence stars. It is shown that the Na excess in a large fraction of yellow supergiants with M greater than or similar to 7-10 M-circle dot can only be understood as a result of mixing of Na between the convective core and the radiative envelope in their main-sequence progenitors. We demonstrate that the vertical turbulent diffusion from the Zahn model could be responsible for this extra mixing.
引用
收藏
页码:1058 / 1067
页数:10
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