A 6.7 GHz Methanol Maser Survey. II. Low Galactic Latitudes

doi:10.3847/1538-4365/ab06fb

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	A 6.7 GHz Methanol Maser Survey. II. Low Galactic Latitudes
	Yang,Kai1,2 ; Chen,Xi1,3,4 ; Shen,Zhi-Qiang 1,4; Li,Xiao-Qiong 1,2; Wang,Jun-Zhi 1,4; Jiang,Dong-Rong 1,4; Li,Juan1,4 ; Dong,Jian1,4 ; Wu,Ya-Jun 1,4; Qiao,Hai-Hua 1,5
刊名	The Astrophysical Journal Supplement Series
	2019-03-20
卷号	241 期号:2
关键词	ISM: molecules masers radio lines: ISM stars: formation
ISSN号	0067-0049
DOI	10.3847/1538-4365/ab06fb
英文摘要	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.
语种	英语
出版者	The American Astronomical Society
WOS记录号	IOP:0067-0049-241-2-AB06FB
内容类型	期刊论文
源URL	[http://119.78.226.72/handle/331011/31883]
专题	中国科学院上海天文台
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).