PMO OpenIR  > 空间目标与碎片观测研究基地
Combination of CN(1-0), HCN(1-0), and HNC(1-0): A possible indicator for a high-mass star formation sequence in the Milky Way
Han, X. H.1,2; Zhou, J. J.1,3; Wang, J. Z.4; Esimbek, J.1,3; Zhang, J. S.5; Wang, N.1,3
2015-04-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume576
AbstractContext. CN, HCN, and HNC have been used to discuss the star formation sequence in galaxies, but recent studies of large samples involving these lines did not yet provide convincing results.
KeywordIsm: Clouds Ism: Molecules
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1051/0004-6361/201423791
WOS KeywordH-II REGIONS ; LUMINOUS INFRARED GALAXIES ; PROTOSTELLAR CANDIDATES ; INTERSTELLAR CLOUDS ; PHYSICAL-PROPERTIES ; CHEMICAL EVOLUTION ; GALACTIC PLANE ; FORMING REGION ; OUTER GALAXY ; DARK CLOUDS
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000357274600066
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Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/16005
Collection空间目标与碎片观测研究基地
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
2.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China
4.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
5.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China
Recommended Citation
GB/T 7714
Han, X. H.,Zhou, J. J.,Wang, J. Z.,et al. Combination of CN(1-0), HCN(1-0), and HNC(1-0): A possible indicator for a high-mass star formation sequence in the Milky Way[J]. ASTRONOMY & ASTROPHYSICS,2015,576.
APA Han, X. H.,Zhou, J. J.,Wang, J. Z.,Esimbek, J.,Zhang, J. S.,&Wang, N..(2015).Combination of CN(1-0), HCN(1-0), and HNC(1-0): A possible indicator for a high-mass star formation sequence in the Milky Way.ASTRONOMY & ASTROPHYSICS,576.
MLA Han, X. H.,et al."Combination of CN(1-0), HCN(1-0), and HNC(1-0): A possible indicator for a high-mass star formation sequence in the Milky Way".ASTRONOMY & ASTROPHYSICS 576(2015).
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