NAOC Open IR
用线性化分离法计算膨胀恒星大气的谱线形成
吴关钱; 黄润乾; 龚志刚
1995
Source Publication天体物理学报
ISSN0253-2379
Volume015Issue:002Pages:163
Abstract本文研究了具有宏观运动的膨胀恒星大气中的转射转移过程,详细介绍如何利用线性化分离法计算运动大气谱线形成,并采用线性化分离法计算了Ori星的Hα线 P Cygni轮廓。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/41445
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
吴关钱,黄润乾,龚志刚. 用线性化分离法计算膨胀恒星大气的谱线形成[J]. 天体物理学报,1995,015(002):163.
APA 吴关钱,黄润乾,&龚志刚.(1995).用线性化分离法计算膨胀恒星大气的谱线形成.天体物理学报,015(002),163.
MLA 吴关钱,et al."用线性化分离法计算膨胀恒星大气的谱线形成".天体物理学报 015.002(1995):163.
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