Neutron-capture element trends in the halo

被引:0
|
作者
Sneden, C [1 ]
Cowan, JJ [1 ]
Truran, JW [1 ]
机构
[1] Univ Texas, Dept Astron, Austin, TX 78712 USA
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In a brief review of abundances neutron-capture elements (Z > 30) in metal-poor halo stars, attention is called to their star-to-star scatter, the dominance of r-process synthesis at lowest metallicities, the puzzle of the lighter members of this element group, and the possibility of a better s-/s-process discriminant.
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页码:179 / 184
页数:6
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