NAOC Open IR
Nova Oph 1994光谱观测研究
姜晓军; 胡景耀
1997
Source Publication天体物理学报
ISSN0253-2379
Volume017Issue:002Pages:175
Abstract用2。16m望远镜及其卡焦光谱仪对Nova Oph 1994进行了一系列的光谱观测,其早期光谱中出现的大量Fell线表明它是一颗Fell型新星,而它的发射线的多峰结构在其它Fell型新星中是不多见的,它们根据得到的光谱和从国际互联网络得的测光资料,讨论了它的光谱特征和演化。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/48085
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
姜晓军,胡景耀. Nova Oph 1994光谱观测研究[J]. 天体物理学报,1997,017(002):175.
APA 姜晓军,&胡景耀.(1997).Nova Oph 1994光谱观测研究.天体物理学报,017(002),175.
MLA 姜晓军,et al."Nova Oph 1994光谱观测研究".天体物理学报 017.002(1997):175.
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