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The large-scale distribution and physical properties of massive star forming regions in the Milky Way
Jarken Esimbek1; Zhou Jianjun1; Zheng Xingwu2
2007
Conference NameAstrophysical Masers and their Environments
Source PublicationIAU Symposium
Volume242
Pages228-229
Conference DateMarch 12-16, 2007
Correspondent Emailjarken@ms.xjb.ac.cn ; xwzheng@nju.edu.cn
Conference PlaceAlice Springs, Australia
Project Number10203003 ; 10073004 ; RCPY200605
Contribution Rank1
AbstractWe are conducting a large survey with the Urumqi 25 m radio telescope to study the distribution and physical properties of massive star forming regions in the Milky Way. We will accomplish this by observing the H110 α hydrogen recombination line at 4.874 GHz and the H 2 CO absorption line at 4830 GHz. These lines are associated with compact HII regions and dense molecular clouds. As a test of the 6 cm spectral line receiving system, we observed the two spectral lines toward massive star forming regions. We plan to study the large scale distribution and physical properties of massive star forming regions in the Milky way.
Funding Organization国家自然科学基金 ; 西部之光
KeywordIsm: Hii Regions Galaxy: Kinematics And Dynamics Galaxy: Structure
Subject Area恒星和恒星物理
DOI10.1017/S1743921307013026
URL查看原文
Funding Project恒星形成与演化研究团组
Language英语
ISBN978-0521-87464-9
ISSN1743-9213
Citation statistics
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/29
Collection射电天文研究室_恒星形成与演化研究团组
科研仪器设备产出_利用南山26米射电望远镜(NSRT)观测数据的文章
Affiliation1.National Astronomical Observatories/Urumqi Observatory, CAS, Urumqi 830011, China
2.Department of Astronomy, Nanjing University, Nanjing 210093, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
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Jarken Esimbek,Zhou Jianjun,Zheng Xingwu. The large-scale distribution and physical properties of massive star forming regions in the Milky Way[C],2007:228-229.
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