A chemodynamical simulation of halo stars in the milky way

被引：0
|
作者：
Nakasato, N. [1 ]
机构：
[1] RIKEN, Wako, Saitama 3510198, Japan
来源：
CRAL-2006 Chemodynamics: From First Stars to Local Galaxies | 2007年 / 24卷
关键词：
D O I：
10.1051/eas:2007044
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this contribution, we present a new chemodynamical model for the early evolution history of the Milky Way with an improved chemical evolution description. Our new approach is based on the chemical evolution model by Tsujimoto et al. (1999). This description enables us to construct a detailed chemical and dynamical model of halo stars in the Milky Way. Especially, we pay a special attention to a relation between chemical properties of halo stars and their kinematics.
引用
收藏
页码：293 / 294
页数：2
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