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题名: Molecular clouds and star formation toward the Galactic plane within 216.25 degrees <= l <= 218.75 degrees and-0.75 degrees. <= b <= 1.25 degrees
作者: Gong, Y.1, 2, 3; Mao, R. Q.1, 2; Fang Min(房敏)1, 2; Zhang, S. B.1, 2; Su, Y.1, 2; Yang Ji(杨戟)1, 2; Jiang, Z. B.1, 2; Xu Ye(徐烨)1, 2; Wang Min(王旻)1, 2; Wang Ying(王英)1, 2; Lu, D. R.1, 2; Sun, J. X.1, 2
刊名: ASTRONOMY & ASTROPHYSICS
出版日期: 2016-04-01
卷号: 588
关键词: surveys ; ISM: clouds ; stars: formation ; radio lines: ISM ; ISM: kinematics and dynamics
DOI: 10.1051/0004-6361/201527334
文章类型: Article
英文摘要: Context. Molecular clouds trace the spiral arms of the Milky Way and all its star forming regions. Large-scale mapping of molecular clouds will provide an approach to understand the processes that govern star formation and molecular cloud evolution.
WOS标题词: Science & Technology ; Physical Sciences
类目[WOS]: Astronomy & Astrophysics
研究领域[WOS]: Astronomy & Astrophysics
关键词[WOS]: INFRARED-DARK CLOUD ; YOUNG STELLAR OBJECTS ; MILKY-WAY ; FORMING REGIONS ; FORMATION RATES ; INTERSTELLAR-MEDIUM ; SUPERNOVA REMNANT ; RADIO ASTRONOMY ; MAGNETIC-FIELDS ; OB-ASSOCIATIONS
收录类别: SCI
项目资助者: National Natural Science Foundation of China (NSFC)(11127903 ; Strategic Priority Research Program of the Chinese Academy of Sciences(XDB09000000) ; NSFC(11203081) ; National Aeronautics and Space Administration ; National Science Foundation ; 11233007 ; 10973040)
语种: 英语
WOS记录号: WOS:000373207800116
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/16199
Appears in Collections:分子云与恒星形成研究团组_期刊论文

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作者单位: 1.Chinese Acad Sci, Purple Mt Observ, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China
3.Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
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