NTSC-IR
A 6.7 GHz Methanol Maser Survey. II. Low Galactic Latitudes
Yang,Kai1,2; Chen,Xi1,3,4; Shen,Zhi-Qiang1,4; Li,Xiao-Qiong1,2; Wang,Jun-Zhi1,4; Jiang,Dong-Rong1,4; Li,Juan1,4; Dong,Jian1,4; Wu,Ya-Jun1,4; Qiao,Hai-Hua1,5
2019-03-20
发表期刊The Astrophysical Journal Supplement Series
ISSN0067-0049
卷号241期号:2
摘要Abstract We report the results of our systematic survey for Galactic 6.7 GHz Class II CH3OH maser emission toward a sample of young stellar objects. The survey was conducted with the Shanghai Tianma Radio Telescope (TMRT). The sample consists of 3348 sources selected from the all-sky Wide-field Infrared Survey Explorer (WISE) point-source catalog. We discussed the selection criteria in detail and the detection results of those at high Galactic latitudes (i.e., ) in a previous paper (Yang et al. 2017). Here, we present the results from the survey of those at low Galactic latitudes, i.e., . Of 1875 selected WISE point sources, 291 positions that were actually associated with 224 sources that were detected with CH3OH maser emission. Among them, 32 are newly detected. A majority of the newly detected sources are associated with bright WISE sources. The majority of the detected sources (209/224?=?93.3%) are quite close to the Galactic Plane ( ) and lie on the inner spiral arms with positive local standard of rest velocities. The detection rate and the color–color distribution of our detection are all matched with our anticipation. Combining with detections from previous surveys, we compile a catalog of 1085 sources with 6.7 GHz CH3OH maser emission in our Galaxy.
关键词ISM: molecules masers radio lines: ISM stars: formation
DOI10.3847/1538-4365/ab06fb
语种英语
WOS记录号IOP:0067-0049-241-2-ab06fb
出版者The American Astronomical Society
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文献类型期刊论文
条目标识符http://210.72.145.45/handle/361003/10739
专题中国科学院国家授时中心
作者单位1.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, People’s Republic of China; yangkai@shao.ac.cn, chenxi@shao.ac.cn, zshen@shao.ac.cn
2.University of Chinese Academy of Sciences, 19A Yuquanlu, Beijing 100049, People’s Republic of China
3.Center for Astrophysics, Guangzhou University, Guangzhou 510006, People’s Republic of China; chenxi@gzhu.edu.cn
4.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, People’s Republic of China
5.National Time Service Center, Chinese Academy of Sciences, Xi’An, Shaanxi, 710600, People’s Republic of China
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Yang,Kai,Chen,Xi,Shen,Zhi-Qiang,et al. A 6.7 GHz Methanol Maser Survey. II. Low Galactic Latitudes[J]. The Astrophysical Journal Supplement Series,2019,241(2).
APA Yang,Kai.,Chen,Xi.,Shen,Zhi-Qiang.,Li,Xiao-Qiong.,Wang,Jun-Zhi.,...&Qiao,Hai-Hua.(2019).A 6.7 GHz Methanol Maser Survey. II. Low Galactic Latitudes.The Astrophysical Journal Supplement Series,241(2).
MLA Yang,Kai,et al."A 6.7 GHz Methanol Maser Survey. II. Low Galactic Latitudes".The Astrophysical Journal Supplement Series 241.2(2019).
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