Solar s-process contributions with GCE model

We study the s-process abundances (A>~90) at the epoch of the solar system formation. Asymptotic giant branch yields are computed with an updated neutron capture network and...本研究针对太阳系形成时期的慢中子俘获过程（s-process）元素丰度（原子量A>约90）展开分析。研究采用更新后的中子俘获网络，对渐近巨星支（Asymptotic Giant Branch, AGB）恒星的元素产额进行计算，并……