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Submillimeter/millimeter observations of the high-mass star forming region IRAS 22506+5944
Xu, Jin-Long1; Wang, Jun-Jie
2010-02-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
Volume10Issue:2Pages:151-158
AbstractThe mapping observations of CO J = 2 - 1, CO J = 3 - 2, (13)CO J = 2 - 1 and (13)CO J = 3 - 2 lines in the direction of IRAS 22506+5944 have been made. The results show that the cores in the J = 2 - 1 transition lines have a similar morphology to those in the J = 3 - 2 transition lines. Bipolar molecular outflows are verified. The prior IRAS 22506+5944 observations indicated that two IRAS sources and three H(2)O masers were located close to the peak position of the core. One of the IRAS sources, may be the driving source of the outflows. In addition, the H(2)O masers may occur in relatively warm environments. The parameters of the dense core and outflow, obtained by the LTE method, indicate that IRAS 22506+5944 is a high-mass star formation region.
KeywordIsm: Jets And Outflows Ism: Kinematics And Dynamics Ism: Molecules Stars: Formation
Indexed BySCI
Language英语
WOS IDWOS:000275349700006
Citation statistics
Cited Times:13[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/7777
Collection射电天文研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.NAOC TU Joint Ctr Astrophys, Lhasa 850000, Peoples R China
Recommended Citation
GB/T 7714
Xu, Jin-Long,Wang, Jun-Jie. Submillimeter/millimeter observations of the high-mass star forming region IRAS 22506+5944[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2010,10(2):151-158.
APA Xu, Jin-Long,&Wang, Jun-Jie.(2010).Submillimeter/millimeter observations of the high-mass star forming region IRAS 22506+5944.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,10(2),151-158.
MLA Xu, Jin-Long,et al."Submillimeter/millimeter observations of the high-mass star forming region IRAS 22506+5944".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 10.2(2010):151-158.
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