Fig. 1.
Channel maps for the 12CO (2–1) emission. Images are shown for 1.3 km s−1 channel bins, spaced 3 km s−1 apart and shifted to zero at the systemic velocity of −9 km s−1. The overlaid white contours correspond to the SO emission, and trace 4, 5, 6, 10, and 14 times the rms value of 0.93 mJy beam−1. In this and all other spatial figures, the x and y axes give the relative RA and Dec in arcseconds from the position of GX Mon, unless otherwise indicated.
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