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Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde II. The Large Magellanic Cloud
Tang, X. D.1,2,3; Henkel, C.1,4; Chen, C. -H. R.1; Menten, K. M.1; Indebetouw, R.5,6; Zheng, X. W.7; Esimbek, J.2,3; Zhou, J. J.2,3; Yuan, Y.2,3; Li, D. L.2,3; He, Y. X.2,3
2017-04-01
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN1432-0746
Volume600Pages:A16
Contribution Rank3
Abstract

Context. The kinetic temperature of molecular clouds is a fundamental physical parameter affecting star formation and the initial mass function. The Large Magellanic Cloud (LMC) is the closest star-forming galaxy with a low metallicity and provides an ideal laboratory for studying star formation in such an environment.

Correspondent Emailxdtang@mpifr-bonn.mpg.de
KeywordStars: Formation Magellanic Clouds Ism: Clouds Ism: Molecules Radio Lines: Ism
SubtypeArticle
DOI10.1051/0004-6361/201630183
WOS HeadingsScience & Technology ; Physical Sciences
URL查看原文
Indexed BySCI
Language英语
WOS KeywordSest Key Program ; Dense Gas ; Nearby Galaxies ; Galactic-center ; Physical-properties ; n 159 ; Interstellar Ammonia ; Starburst Galaxies ; Submillimeter Line ; Isotope Ratios
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000400754000129
Funding OrganizationNational Natural Science Foundation of China(11433008, 11373062) ; Program of the Light in China's Western Region (LCRW)(XBBS201424) ; Chinese Academy of Sciences(2013T2J0057)
Citation statistics
Cited Times:9[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/1631
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
Corresponding AuthorTang, X. D.
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.Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA
6.Univ Virginia, Charlottesville, VA 22903 USA
7.Nanjing Univ, Dept Astron, Nanjing, Jiangsu, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Tang, X. D.,Henkel, C.,Chen, C. -H. R.,et al. Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde II. The Large Magellanic Cloud[J]. ASTRONOMY & ASTROPHYSICS,2017,600:A16.
APA Tang, X. D..,Henkel, C..,Chen, C. -H. R..,Menten, K. M..,Indebetouw, R..,...&He, Y. X..(2017).Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde II. The Large Magellanic Cloud.ASTRONOMY & ASTROPHYSICS,600,A16.
MLA Tang, X. D.,et al."Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde II. The Large Magellanic Cloud".ASTRONOMY & ASTROPHYSICS 600(2017):A16.
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