中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A new interpretation of the bipolar HII region S106 from HCN J=3-2 mapping observations

文献类型:期刊论文

作者Qin, SL; Wang, JJ; Zhao, G; Miller, M
刊名CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
出版日期2005-02-01
卷号5期号:1页码:1-5
关键词ISM : clouds nebulae : HII region star : formation individual : S106
英文摘要The first mapping observations of the bipolar HII region S106 in HCN J = 3 - 2 line were made by KOSMA submillimeter telescope in April, 2004. The results show that there is a bipolar outflow centered on the high-mass star S106 IRS4 and that the flat structure of molecular cloud core is perpendicular to the axis of the outflow. This image roughly corresponds to the optical image where a dark lane bisects the bipolar HII region. Together with the optical, infrared and radio data, we conclude that the central UC HII region and molecular outflow formed before the two lobes of the bipolar HII region, and that a neutral disk is responsible for the bipolar HII region and the outflow.
收录类别SCI
语种英语
WOS记录号WOS:000228398900001
源URL[http://ir.bao.ac.cn/handle/114a11/7010]  
专题国家天文台_光学天文研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Univ Cologne, Inst Phys, D-50937 Cologne, Germany
推荐引用方式
GB/T 7714
Qin, SL,Wang, JJ,Zhao, G,et al. A new interpretation of the bipolar HII region S106 from HCN J=3-2 mapping observations[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2005,5(1):1-5.
APA Qin, SL,Wang, JJ,Zhao, G,&Miller, M.(2005).A new interpretation of the bipolar HII region S106 from HCN J=3-2 mapping observations.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,5(1),1-5.
MLA Qin, SL,et al."A new interpretation of the bipolar HII region S106 from HCN J=3-2 mapping observations".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 5.1(2005):1-5.

入库方式: OAI收割

来源:国家天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。