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钡星重元素丰度的参数化研究
引用本文:张彩霞,刘俊红. 钡星重元素丰度的参数化研究[J]. 江苏科技大学学报(社会科学版), 2009, 23(4): 373-376
作者姓名:张彩霞  刘俊红
作者单位:石家庄学院,物理系,河北,石家庄,050035;石家庄学院,物理系,河北,石家庄,050035
基金项目:国家自然科学基金资助项目 
摘    要:提出了一种计算钡星重元素丰度的参数化方法,利用此方法对7颗钡星进行了参数化研究,计算出这些星的最佳拟合参数及其重元素丰度.对核合成参数进行了讨论,将重元素丰度的计算结果与观测值进行了比较,结果符合较好,证明了文中提出的模型的有效性.

关 键 词:钡星  参数化模型  AGB星  核合成

Parametric model of heavy element abundance in barium stars
Zhang Caixia,Liu Junhong. Parametric model of heavy element abundance in barium stars[J]. Journal of Jiangsu University of Science and Technology(Natural Science Edition), 2009, 23(4): 373-376
Authors:Zhang Caixia  Liu Junhong
Affiliation:(Department of Physics, Shijiazhuang College, Shijiazhuang Hebei 050035, China)
Abstract:To calulate heavy element abundances of barium stars, a new parametric model was proposed in this paper. Based on the model, appropriate fitting parameters and heavy element abundances of 7 barium stars were studied, and nucleosynthesis parameters were discussed. The computing results of heavy element abundances from the model were basically agreeable with these from observations. This means the developed model is valid.
Keywords:barium stars  parametric model  AGB-stars  nucleosynthesis
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