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A H2CO and H110 alpha survey of H II regions with the 25-m radio telescope of Nanshan Station
Du, Z. M.1,2; Zhou, J. J.1,3; Esimbek, J.1,3; Han, X. H.1,2; Zhang, C. P.1,2
2011-08-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume532Pages:A127
Contribution Rank1
AbstractContext. Accurate distances are necessary for determining the physical properties of massive star-formation regions and the structure of our Galaxy. One way to approach these studies is by determining the kinematic distances of H II regions.
KeywordGalaxy: Structure h Ii Regions Ism: Molecules Radio Lines: Ism
SubtypeArticle
DOI10.1051/0004-6361/201116506
WOS HeadingsScience & Technology ; Physical Sciences
Indexed BySCI
Language英语
WOS KeywordMASSIVE STAR-FORMATION ; ULTRACOMPACT HII-REGIONS ; CENTER MOLECULAR CLOUDS ; MILKY-WAY GALAXY ; DISTANCE AMBIGUITIES ; RECOMBINATION LINES ; GALACTIC STRUCTURE ; FORMALDEHYDE ; RESOLUTION ; CALIBRATORS
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000293942700026
Citation statistics
Cited Times:9[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/845
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
研究生学位论文
其它
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
2.Chinese Acad Sci, Grad Univ, Beijing 100080, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Du, Z. M.,Zhou, J. J.,Esimbek, J.,et al. A H2CO and H110 alpha survey of H II regions with the 25-m radio telescope of Nanshan Station[J]. ASTRONOMY & ASTROPHYSICS,2011,532:A127.
APA Du, Z. M.,Zhou, J. J.,Esimbek, J.,Han, X. H.,&Zhang, C. P..(2011).A H2CO and H110 alpha survey of H II regions with the 25-m radio telescope of Nanshan Station.ASTRONOMY & ASTROPHYSICS,532,A127.
MLA Du, Z. M.,et al."A H2CO and H110 alpha survey of H II regions with the 25-m radio telescope of Nanshan Station".ASTRONOMY & ASTROPHYSICS 532(2011):A127.
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