s-process abundances in halo stars
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The chemical evolution history of slow neutron-capture elements in the Milky Way is still a matter of debate, especially in the metal-poor regime ([Fe/H]<-1). Based on...
银河系中慢中子俘获元素（slow neutron-capture elements）的化学演化历程至今仍存在学术争议，尤其是在贫金属区域（metal-poor regime，即[Fe/H]<-1）。基于
