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题名: N131: A dust bubble born from the disruption of a gas filament
作者: Zhang, Chuan-Peng1, 2, 6, 7; Li, Guang-Xing2, 3; Wyrowski, Friedrich2; Wang, Jun-Jie1, 6; Yuan, Jing-Hua1; Xu, Jin-Long1, 6; Gong, Yan2, 4, 5, 7; Yeh, Cosmos C.2; Menten, Karl M.2
刊名: ASTRONOMY & ASTROPHYSICS
出版日期: 2016
卷号: 585
关键词: infrared: ISM ; stars: formation ; ISM: bubbles ; ISM: clouds
DOI: 10.1051/0004-6361/201526296
文章类型: Article
英文摘要: Context. OB-type stars have strong ionizing radiation and drive energetic winds. The ultraviolet radiation from ionizing stars may heat dust and ionize gas to sweep up an expanding bubble shell. This shell may be the result of feedback leading to a new generation of stars.
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 ; H-II REGIONS ; STAR-FORMATION ; INTERSTELLAR BUBBLES ; MILKY-WAY ; GALACTIC PLANE ; HIERARCHICAL FRAGMENTATION ; MOLECULAR CLOUDS ; MASSIVE STARS ; DATA RELEASE
收录类别: SCI
项目资助者: MPG-CAS Joint Doctoral Promotion Program (DPP) ; National Key Basic Research Program of China (973 Program)(2015CB857100) ; National Natural Science Foundation of China(11363004 ; 11403042)
语种: 英语
WOS记录号: WOS:000369710300124
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/16143
Appears in Collections:南极天文中心_期刊论文

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作者单位: 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
3.Univ Observ Munich, Scheinerstr 1, D-81679 Munich, Germany
4.Chinese Acad Sci, Purple Mt Observ, 2 West Beijing Rd, Nanjing 210008, Peoples R China
5.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Peoples R China
6.NAOC TU Joint Ctr Astrophys, Lhasa 850000, Peoples R China
7.Univ Chinese Acad Sci, Beijing 100080, Peoples R China
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