Chemical Tagging of Kinematic Stellar Groups in the Milky Way Disk

被引：0
|
作者：
Nordstrom, B. [1 ]
Stonkute, E. [2 ]
Tautvaisiene, G. [2 ]
Zenoviene, R. [2 ]
机构：
[1] Niels Bohr Inst, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark
[2] Vilnius State Univ, Inst Theoret Phys & Astron, LT-01108 Vilnius, Lithuania
来源：
GALACTIC ARCHAEOLOGY: NEAR-FIELD COSMOLOGY AND THE FORMATION OF THE MILKY WAY | 2012年 / 458卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present a progress report on a chemical abundance analysis of two kinematic stellar groups in the Galactic disk, suspected to be relicts of disrupted satellites. Their origin remains an open question, but chemical tagging is providing new clues.
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页码：235 / +
页数：2
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