Abundances as tracers of the formation and evolution of (Dwarf) galaxies

被引：0
|
作者：
Tolstoy, E. [1 ]
机构：
[1] Univ Groningen, Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
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_73
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This aims to be an overview of what detailed observations of individual stars in nearby dwarf galaxies may teach us about galaxy evolution. This includes some early results from the DART (Dwarf Abundances and Radial velocity Team) Large Programme at ESO. This project has used 2.2m/WFI and VLT/FLAMES to obtain spectra of large samples of individual stars in nearby dwarf spheroidal galaxies and determine accurate abundances and kinematics. These results can be used to trace the formation and evolution of nearby galaxies from the earliest times to the present.
引用
收藏
页码：213 / 218
页数：6
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