A 6.7 GHz Methanol Maser Survey II. Low Galactic Latitudes

We report the results of our systematic survey for Galactic 6.7 GHz Class II CH_3OH 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 have discussed the selection criteria in detail and the detection results of those at high Galactic latitudes (i.e. |b|> 2^∘) in a previous paper (paper I). Here, we present the results from the survey of those at low Galactic latitudes, i.e. |b|<2^∘. Of 1875 selected WISE point sources, 291 positions that were actually associated with 224 sources were detected with CH_3OH maser emission. Among them, 32 are newly detected. 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 (|b|<1^∘) and lie on the inner spiral arms with positive LSR velocities. 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 catalogue of 1085 sources with 6.7 GHz CH_3OH maser emission in our Galaxy.