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ATLASGAL-selected massive clumps in the inner Galaxy VI. Kinetic temperature and spatial density measured with formaldehyde
Tang, X. D.1,2,3; Henkel, C.1,4; Wyrowski, F.1; Giannetti, A.1,5,6; Menten, K. M.1; Csengeri, T.1; Leurini, S.1,7; Urquhart, J. S.1,8; Koenig, C.1; Guesten, R.1; Lin, Y. X.1; Zheng, X. W.9; Esimbek, J.2,3; Zhou, J. J.2,3
2018-03-15
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN1432-0746
Volume611Pages:A6
Contribution Rank2
Abstract

Context. Formaldehyde (H2CO) is a reliable tracer to accurately measure the physical parameters of dense gas in star-forming regions.

KeywordStars: Formation Stars: Massive Ism: Clouds Ism: Molecules Ism: Abundances Radio Lines: Ism
SubtypeArticle
DOI10.1051/0004-6361/201732168
WOS HeadingsScience & Technology ; Physical Sciences
URL查看原文
Indexed BySCI
Language英语
WOS KeywordStar-forming Regions ; Young Stellar Objects ; Molecular Clouds ; Galactic-center ; Physical-properties ; Complete Sample ; Infall Motions ; Cepheus Clouds ; Survey Ammonia ; Iras Sources
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000427914900001
Funding OrganizationNational Natural Science Foundation of China(11433008, 11373062) ; Program of the Light in China's Western Region (LCRW)(XBBS201424) ; Deutsche Forschungsgemeinschaft (DFG). ; Chinese Academy of Sciences President's International Fellowship Initiative(2017VMA0005)
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Cited Times:9[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/1903
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
Affiliation1.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Peoples R China
4.King Abdulaziz Univ, Astron Dept, POB 80203, Jeddah 21589, Saudi Arabia
5.INAF Ist Radioastron, Via P Gobetti 101, I-40129 Bologna, Italy
6.Italian ALMA Reg Ctr, Via P Gobetti 101, I-40129 Bologna, Italy
7.INAF Osservatorio Astron Cagliari, Via Sci 5, I-09047 Selargius, CA, Italy
8.Univ Kent, Sch Phys Sci, Ingram Bldg, Canterbury CT2 7NH, Kent, England
9.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Tang, X. D.,Henkel, C.,Wyrowski, F.,et al. ATLASGAL-selected massive clumps in the inner Galaxy VI. Kinetic temperature and spatial density measured with formaldehyde[J]. ASTRONOMY & ASTROPHYSICS,2018,611:A6.
APA Tang, X. D..,Henkel, C..,Wyrowski, F..,Giannetti, A..,Menten, K. M..,...&Zhou, J. J..(2018).ATLASGAL-selected massive clumps in the inner Galaxy VI. Kinetic temperature and spatial density measured with formaldehyde.ASTRONOMY & ASTROPHYSICS,611,A6.
MLA Tang, X. D.,et al."ATLASGAL-selected massive clumps in the inner Galaxy VI. Kinetic temperature and spatial density measured with formaldehyde".ASTRONOMY & ASTROPHYSICS 611(2018):A6.
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