PMO OpenIR  > 南极天文中心
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
Source PublicationASTRONOMY & ASTROPHYSICS
Volume585
AbstractContext. 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.
KeywordInfrared: Ism Stars: Formation Ism: Bubbles Ism: Clouds
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1051/0004-6361/201526296
WOS KeywordINFRARED DARK CLOUD ; H-II REGIONS ; STAR-FORMATION ; INTERSTELLAR BUBBLES ; MILKY-WAY ; GALACTIC PLANE ; HIERARCHICAL FRAGMENTATION ; MOLECULAR CLOUDS ; MASSIVE STARS ; DATA RELEASE
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000369710300124
Citation statistics
Cited Times:10[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/16143
Collection南极天文中心
Affiliation1.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
Recommended Citation
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).
Files in This Item:
File Name/Size DocType Version Access License
2016025.pdf(2364KB) 开放获取Apache LicenseView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Zhang, Chuan-Peng]'s Articles
[Li, Guang-Xing]'s Articles
[Wyrowski, Friedrich]'s Articles
Baidu academic
Similar articles in Baidu academic
[Zhang, Chuan-Peng]'s Articles
[Li, Guang-Xing]'s Articles
[Wyrowski, Friedrich]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Zhang, Chuan-Peng]'s Articles
[Li, Guang-Xing]'s Articles
[Wyrowski, Friedrich]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 2016025.pdf
Format: Adobe PDF
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.