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N131: A dust bubble born from the disruption of a gas filament
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
2016
发表期刊ASTRONOMY & ASTROPHYSICS
卷号585
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.
文章类型Article
关键词Infrared: Ism Stars: Formation Ism: Bubbles Ism: Clouds
WOS标题词Science & Technology ; Physical Sciences
DOI10.1051/0004-6361/201526296
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
语种英语
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)
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000369710300124
引用统计
文献类型期刊论文
条目标识符http://libir.pmo.ac.cn/handle/332002/16143
专题南极天文中心
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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Zhang, Chuan-Peng,Li, Guang-Xing,Wyrowski, Friedrich,et al. N131: A dust bubble born from the disruption of a gas filament[J]. ASTRONOMY & ASTROPHYSICS,2016,585.
APA Zhang, Chuan-Peng.,Li, Guang-Xing.,Wyrowski, Friedrich.,Wang, Jun-Jie.,Yuan, Jing-Hua.,...&Menten, Karl M..(2016).N131: A dust bubble born from the disruption of a gas filament.ASTRONOMY & ASTROPHYSICS,585.
MLA Zhang, Chuan-Peng,et al."N131: A dust bubble born from the disruption of a gas filament".ASTRONOMY & ASTROPHYSICS 585(2016).
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