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Fe离子M壳层不可分辨跃迁系不透明度研究
董富通; 王菲鹿; 仲佳勇; 赵刚
2012
Source Publication物理学报
ISSN1000-3290
Volume061Issue:016Pages:163201
Abstract在活动星系核吸收光谱中存在着一种重要的吸收特征-铁元素的M壳层不可分辨跃迁系吸收谱,认识这种特征对于活动星系核区的物理性质的研究具有重要的意义.利用细致谱线模型,对实验室中获得的吸收谱进行了理论计算和分析,较好地重现了实验结果中主要的吸收结构,同时计算了温度为10-50eV的预测吸收谱,用于活动星系核光谱的研究.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/47651
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
董富通,王菲鹿,仲佳勇,等. Fe离子M壳层不可分辨跃迁系不透明度研究[J]. 物理学报,2012,061(016):163201.
APA 董富通,王菲鹿,仲佳勇,&赵刚.(2012).Fe离子M壳层不可分辨跃迁系不透明度研究.物理学报,061(016),163201.
MLA 董富通,et al."Fe离子M壳层不可分辨跃迁系不透明度研究".物理学报 061.016(2012):163201.
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