NAOC Open IR
相接双星大熊座AW的基本参量
刘清耀; 张运林; 王毕; 杨毓兰
1990
Source Publication天体物理学报
ISSN0253-2379
Volume10Issue:1Pages:42
Abstract根据作者提出的确定食双星基本参量的一个新方法,由光变极小时刻求出了相接双星大熊座AW的基本参量。证实了Rensing等人为了矫正相接双星邻近效应引起的谱线轮廓畸变所提出的模型对该双星的适用性;同时也证实了Mochnaski提出的计算相接双星质量的理论模型对该双星的适用性。另外还确认了大熊座AW是一个已演化的零龄相接双星。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/39925
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
刘清耀,张运林,王毕,等. 相接双星大熊座AW的基本参量[J]. 天体物理学报,1990,10(1):42.
APA 刘清耀,张运林,王毕,&杨毓兰.(1990).相接双星大熊座AW的基本参量.天体物理学报,10(1),42.
MLA 刘清耀,et al."相接双星大熊座AW的基本参量".天体物理学报 10.1(1990):42.
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