中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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
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.
收录类别SCI
语种英语
WOS记录号WOS:000369710300124
源URL[http://ir.bao.ac.cn/handle/114a11/5435]  
专题国家天文台_射电天文研究部
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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来源:国家天文台

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