Fig. 2.
Left: SO (5−4) line emission obtained by binning the velocity channels between −11.4 and −4.9 km s−1, chosen so as to emphasise the morphology of the weak ring and arc-like emission. Right: composite ACS/HST image of GX Mon in the F606W and F814W bands, overlaid with the SO (5–4) emission from the left panel (black contours). The white arrow indicates the direction of the proper motion as taken from Gaia DR2 via Simbad.
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