Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde II. The Large Magellanic Cloud

doi:10.1051/0004-6361/201630183

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	Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde II. The Large Magellanic Cloud
	Tang, X. D.5,6,7 ; He, Y. X.5,6 ; Li, D. L.5,6 ; Yuan, Y.5,6 ; Zhou, J. J.5,6 ; Esimbek, J.5,6 ; Zheng, X. W.2; Indebetouw, R.1,3; Menten, K. M.7; Chen, C. -H. R.7
刊名	ASTRONOMY & ASTROPHYSICS
	2017-04-01
卷号	600 页码:A16
关键词	Stars: Formation Magellanic Clouds Ism: Clouds Ism: Molecules Radio Lines: Ism
ISSN号	1432-0746
DOI	10.1051/0004-6361/201630183
产权排序	3
文献子类	Article
英文摘要	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.
URL标识	查看原文
WOS关键词	Sest Key Program ; Dense Gas ; Nearby Galaxies ; Galactic-center ; Physical-properties ; n 159 ; Interstellar Ammonia ; Starburst Galaxies ; Submillimeter Line ; Isotope Ratios
WOS研究方向	Astronomy & Astrophysics
语种	英语
WOS记录号	WOS:000400754000129
资助机构	National Natural Science Foundation of China(11433008, 11373062) ; Program of the Light in China's Western Region (LCRW)(XBBS201424) ; Chinese Academy of Sciences(2013T2J0057)
内容类型	期刊论文
源URL	[http://ir.xao.ac.cn/handle/45760611-7/1631]
专题	恒星形成与演化研究团组新疆天文台_射电天文研究室
通讯作者	Tang, X. D.
作者单位	1.Univ Virginia, Charlottesville, VA 22903 USA 2.Nanjing Univ, Dept Astron, Nanjing, Jiangsu, Peoples R China 3.Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA 4.King Abdulaziz Univ, Astron Dept, POB 80203, Jeddah 21589, Saudi Arabia 5.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Peoples R China 6.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 7.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
推荐引用方式 GB/T 7714	Tang, X. D.,He, Y. X.,Li, D. L.,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..,He, Y. X..,Li, D. L..,Yuan, Y..,Zhou, J. J..,...&Henkel, C..(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.