A set of samples of 13 massive star-forming cores were observed in SiO (2-1), CH_3_OH (2-1) and C^34^S (2-1) thermal lines. Nine of these cores were detected in all three lines. Among the nine SiO detections, three were new detections, and relatively faint. Most of the lines have wide wings, which might be interpreted as the evidence of ongoing energetic outflows in the cores.
Cone search capability for table J/other/ChA+A/36.238/table14 (Observed samples and the RMS levels of each line after channel smoothing (table1) and column density and abundance (table4))
