N131: A dust bubble born from the disruption of a gas filament

	N131: A dust bubble born from the disruption of a gas filament
	Zhang, Chuan-Peng 1,2,6,7; Li, Guang-Xing 2,3; Wyrowski, Friedrich 2; Wang, Jun-Jie 1,6; Yuan, Jing-Hua 1; Xu, Jin-Long 1,6; Gong, Yan 2,4,5,7; Yeh, Cosmos C.2; Menten, Karl M.2
刊名	ASTRONOMY & ASTROPHYSICS
	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
内容类型	期刊论文
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).