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Tianma 65-m telescope detection of new OH maser features towards the water fountain source IRAS 18286-0959
Chen, Xi1,2,3; Shen, Zhi-Qiang1,3; Li, Xiao-Qiong1,4; Yang, Kai1,4; Nakashima, Jun-ichi5; Wu, Ya-Jun1,3; Zhao, Rong-Bin1,3; Li, Juan1,3; Wang, Jun-Zhi1,3; Jiang, Dong-Rong1,3; Wang, Jin-Qing1,3; Li, Bin1,3; Zhong, Wei-Ye1,3; Yung, Bosco H. K.6
2017-07-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume468Issue:3Pages:3602-3606
Corresponding AuthorChen, Xi(chenxi@shao.ac.cn) ; Shen, Zhi-Qiang(zshen@shao.ac.cn)
AbstractWe report the results of the OH maser observation towards the water fountain source IRAS 18286-0959 using the newly built Shanghai Tianma 65-m Radio Telescope. We observed the three OH ground state transition lines at frequencies of 1612, 1665 and 1667 MHz. Comparing with the spectra of previous observations, we find new maser spectral components at velocity channels largely shifted from the systemic velocity: the velocity offsets of the newly found components lie in the range 20-40 km s(-1) with respect to the systemic velocity. Besides maser variability, another possible interpretation for the newly detected maser features is that part of the molecular gas in the circumstellar envelope is accelerated. The acceleration is probably caused by the passage of a high-velocity molecular jet, which has been detected in previous Very Long Baseline Interferometry observations in the H2O maser line.
Keywordmasers stars: AGB and post-AGB ISM: molecules radio lines: ISM
DOI10.1093/mnras/stx622
WOS KeywordASYMPTOTIC GIANT BRANCH ; CIRCUMSTELLAR ENVELOPES ; PLANETARY-NEBULAE ; STARS ; JETS ; IDENTIFICATION ; EMISSION ; OUTFLOWS ; DISTANCE ; OBJECTS
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000402808700084
PublisherOXFORD UNIV PRESS
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/23001
Collection中国科学院紫金山天文台
Corresponding AuthorChen, Xi; Shen, Zhi-Qiang
Affiliation1.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
2.GuangZhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China
4.Univ Chinese Acad Sci, 19A Yuquanlu, Beijing 100049, Peoples R China
5.Ural Fed Univ, Dept Astron & Geodesy, Lenin Ave 51, Ekaterinburg 620000, Russia
6.N Copernicus Astron Ctr, Rabianska 8, PL-87100 Torun, Poland
Recommended Citation
GB/T 7714
Chen, Xi,Shen, Zhi-Qiang,Li, Xiao-Qiong,et al. Tianma 65-m telescope detection of new OH maser features towards the water fountain source IRAS 18286-0959[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,468(3):3602-3606.
APA Chen, Xi.,Shen, Zhi-Qiang.,Li, Xiao-Qiong.,Yang, Kai.,Nakashima, Jun-ichi.,...&Yung, Bosco H. K..(2017).Tianma 65-m telescope detection of new OH maser features towards the water fountain source IRAS 18286-0959.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,468(3),3602-3606.
MLA Chen, Xi,et al."Tianma 65-m telescope detection of new OH maser features towards the water fountain source IRAS 18286-0959".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 468.3(2017):3602-3606.
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