3D hydrodynamical Simulations of convection in red-giants stellar atmospheres

被引：1
|
作者：
Collet, R. [1 ]
Asplund, M. [2 ]
Trampedach, R. [2 ]
机构：
[1] Uppsala Univ, Dept Astron & Space Phys, BOX 515, SE-75120 Uppsala, Sweden
[2] Australian Natl Univ Mount Stromlo Observ, Res Sch Astron & Astrophys, Weston, ACT ACT 2611, Australia
来源：
CHEMICAL ABUNDANCES AND MIXING IN STARS IN THE MILKY WAY AND ITS SATELLITES | 2006年
关键词：
D O I：
10.1007/978-3-540-34136-9_98
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present preliminary results of 3D hydrodynamical simulations of surface convection in red giants stars. We investigate the main differences between static 1D and 3D time-dependent model stellar atmospheres of red giants for a range of metallicities between solar and [Fe/H] = -3 focusing in particular on the impact of 3D spectral line formation on the derivation of stellar abundances.
引用
收藏
页码：306 / +
页数：2
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