Abundance ratios in Galactic metal-poor stars

被引：0
|
作者：
Ryan, SG [1 ]
机构：
[1] Open Univ, Dept Phys, Milton Keynes MK7 6AA, Bucks, England
来源：
EVOLUTION OF THE MILKY WAY: STARS VERSUS CLUSTERS | 2000年 / 255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：
Metal-poor stars provide information on the characteristics and chemical evolution of the halo population of the Galaxy, the first epoch of star formation and Galaxy formation (not just locally but with relevance to high-redshift objects), and big bang nucleosynthesis. This paper looks at recent developments in this subject. A more comprehensive review can be found elsewhere (Ryan 2000).
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页码：15 / 26
页数：12
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