中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
High velocity gas in S241 and IRAS 19529+2704

文献类型:期刊论文

作者Wu, YF; Yang, CY; Li, YX
刊名CHINESE ASTRONOMY AND ASTROPHYSICS
出版日期1999
卷号23期号:1页码:6-10
关键词ISM jet and outflow star formation
英文摘要We have studied S241 and IRAS 19529 + 2704 by mapping the J = 1 - 0 transition of (CO)-C-12. High-velocity gas is found in both regions, and is identified as new outflows. The physical properties of the outflows such as size, mass and mechanical momentum are derived, and the characteristics of the driving source are analyzed. A large scale rotation with an angular velocity of omega similar to 0.48 x 10(-14)/s is measured in S241. The results suggest that they are active massive star-forming regions, and the massive young stellar objects are the driving source of the outflows.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]OUTFLOWS ; CLOUDS
收录类别SCI
语种英语
WOS记录号WOS:000082340600002
源URL[http://119.78.226.72/handle/331011/28318]  
专题上海天文台_星系宇宙学重点实验室
作者单位1.Peking Univ, Dept Geophys, Beijing 100871, Peoples R China
2.Beijing Astrophys Ctr, Beijing 100871, Peoples R China
3.Chinese Acad Sci, Shanghai Observ, Shanghai 200030, Peoples R China
推荐引用方式
GB/T 7714
Wu, YF,Yang, CY,Li, YX. High velocity gas in S241 and IRAS 19529+2704[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,1999,23(1):6-10.
APA Wu, YF,Yang, CY,&Li, YX.(1999).High velocity gas in S241 and IRAS 19529+2704.CHINESE ASTRONOMY AND ASTROPHYSICS,23(1),6-10.
MLA Wu, YF,et al."High velocity gas in S241 and IRAS 19529+2704".CHINESE ASTRONOMY AND ASTROPHYSICS 23.1(1999):6-10.

入库方式: OAI收割

来源:上海天文台

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