NAOC Open IR
短周期食双星V361 Lyr和近相接的不接双星
方明骏; 翟迪生
1995
Source Publication天文学报
ISSN0001-5245
Volume036Issue:001Pages:37
Abstract短周期食双星V361Lyr(p=0.3096天)可能是观测到的最短周期的由非简并天体且成的近相接双星,本文采用Kaluzny1989年观测到的V和I光变曲线进行了详细的测光分析。考虑到次子星上由于吸积而引起热斑在径度方向的可能延伸效应,而采用了多热斑模型近似,结果取得了对观测到的畸变光变曲线的很好的拟合。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/47076
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
方明骏,翟迪生. 短周期食双星V361 Lyr和近相接的不接双星[J]. 天文学报,1995,036(001):37.
APA 方明骏,&翟迪生.(1995).短周期食双星V361 Lyr和近相接的不接双星.天文学报,036(001),37.
MLA 方明骏,et al."短周期食双星V361 Lyr和近相接的不接双星".天文学报 036.001(1995):37.
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