N131: A dust bubble born from the disruption of a gas filament
文献类型:期刊论文
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
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出版日期 | 2016 |
卷号 | 585 |
关键词 | infrared: ISM stars: formation ISM: bubbles ISM: clouds |
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 |
语种 | 英语 |
WOS记录号 | WOS:000369710300124 |
源URL | [http://libir.pmo.ac.cn/handle/332002/16143] ![]() |
专题 | 紫金山天文台_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 |
推荐引用方式 GB/T 7714 | 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). |
入库方式: OAI收割
来源:紫金山天文台
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