Properties of the ¹²CO (J = 2−1) emission towards G 350.0-2.0. Left: emission lines for a selection of regions (labelled in the right-hand-side maps) in G 350.0-2.0. The asymmetrical wings in regions 5 and 6 hint at the possibility of interaction, but there seems to be no evidence of shocks from broadened lines in any of the regions. Right: best-fit amplitude (top) and standard deviation (bottom) after fitting a Gaussian function to each pixel in the data cube. The lines in red on the amplitude plot correspond to the two position-velocity slices shown in Fig. 10. The overlaid contours are from the 88 MHz GLEAM image of G 350.0-2.0 (Hurley-Walker et al. 2019).