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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
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ISSN | 0067-0049 |
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 |
DOI | 10.3847/1538-4365/ab06fb |
语种 | 英语 |
WOS记录号 | IOP:0067-0049-241-2-ab06fb |
出版者 | The American Astronomical Society |
引用统计 | |
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 |
推荐引用方式 GB/T 7714 | 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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