Metal-poor stars spectroscopy. II
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Models of post-main sequence stellar evolution of VandenBerg & Bell have been applied to determine spectroscopic masses and distances for metal-poor stars. Careful...
VandenBerg与Bell提出的主序后恒星演化（post-main sequence stellar evolution）模型已被用于测定贫金属星（metal-poor stars）的光谱质量（spectroscopic masses）与距离。严谨的……
