Carbon-enhanced metal-poor (CEMP) star abundances

We investigate anew the distribution of absolute carbon abundance, A(C)=log{epsilon}(C), for carbon-enhanced metal-poor (CEMP) stars in the halo of the Milky Way, based on...我们基于未完整给出的研究基础，重新考察了银河系银晕中富碳贫金属（carbon-enhanced metal-poor, CEMP）恒星的绝对碳丰度$A(C)=logvarepsilon(C)$的分布情况。