A 6 cm VLA‐A contour map is shown overlaid on the Hα HST image of the core. The asterisk marks the position of the star detected by the HST and the cross the possible MERLIN point source, shown here to be coincident with the VLA‐A maximum and the nebular knot located 0﹩\farcs﹩34 south of the central star. The linear VLA‐A 6 cm contour intervals are evenly spaced between 30 and 110 μJy. The half‐power beamwidth of the VLA observations is 0﹩\farcs﹩9.