摘要
利用太阳系的重核素丰度,结合贫金属星重元素丰度的观测值及星系化学演化的计算结果,计算了不同金属丰度恒星三种典型重元素丰度的s-过程、r-过程贡献的相对比例。
Based on the solar system heavy nuclicle abudances ,with the observed abundances of heavy elements in metal-poor stars and the conclusions of the galactic chemical evolution,the relative contribution proportions of the s-process and the r-process abundances of three heavy elements in metal-poor stars with various metallicity are determined.
出处
《石家庄学院学报》
1999年第2期52-54,共3页
Journal of Shijiazhuang University
关键词
贫金属星
重元素
丰度
metal-poor stars
heavey-element
abundance