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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
Volume576Pages:A131
Contribution Rank1
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
SubtypeArticle
DOI10.1051/0004-6361/201423791
WOS HeadingsScience & Technology ; Physical Sciences
Indexed BySCI
Language英语
WOS KeywordH-II REGIONS ; LUMINOUS INFRARED GALAXIES ; PROTOSTELLAR CANDIDATES ; INTERSTELLAR CLOUDS ; PHYSICAL-PROPERTIES ; CHEMICAL EVOLUTION ; GALACTIC PLANE ; FORMING REGION ; OUTER GALAXY ; DARK CLOUDS
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000357274600066
Citation statistics
Cited Times:3[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/875
Collection射电天文研究室_恒星形成与演化研究团组
射电天文研究室
应用天文研究室
其它
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
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
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:A131.
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,A131.
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):A131.
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