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Spectral Classification of Galaxies and Identification of Galactic H ii Regions Based on LAMOST Spectral Line Features
Wang,Li-Li1,2,3
2019-05-21
Source PublicationPublications of the Astronomical Society of the Pacific
ISSN0004-6280
Volume131Issue:1001
Keywordcatalogs galaxies: statistics galaxies: stellar content H ii regions ISM: abundances techniques: spectroscopic
DOI10.1088/1538-3873/ab1e7d
Language英语
WOS IDIOP:0004-6280-131-1001-ab1e7d
PublisherThe Astronomical Society of the Pacific
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Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/28860
Collection中国科学院国家天文台
Affiliation1.School of Information Management, Dezhou University, Dezhou 253023, People’s Republic of China; jsjxwll@126.com
2.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China
3.Institute for Astronomical Science, Dezhou University, Dezhou 253023, People’s Republic of China
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Wang,Li-Li. Spectral Classification of Galaxies and Identification of Galactic H ii Regions Based on LAMOST Spectral Line Features[J]. Publications of the Astronomical Society of the Pacific,2019,131(1001).
APA Wang,Li-Li.(2019).Spectral Classification of Galaxies and Identification of Galactic H ii Regions Based on LAMOST Spectral Line Features.Publications of the Astronomical Society of the Pacific,131(1001).
MLA Wang,Li-Li."Spectral Classification of Galaxies and Identification of Galactic H ii Regions Based on LAMOST Spectral Line Features".Publications of the Astronomical Society of the Pacific 131.1001(2019).
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