Fig. 1

Images of the cometary UCHII G028.6869+00.1770. Top panel: CORNISH 6 cm image with overplotted GLIMPSE 8 micron contours, with the corresponding GLIMPSE image (middle panel), with overplotted radio contours. The morphology at both wavelengths is in very good agreement, and there is excellent positional coincidence between the two catalogues, allowing reliable source identification. The BOLOCAM image (bottom panel) shows a bright unresolved source at 1.1 mm coincident with G028.6869+00.1770 (the source position is marked by a white cross).
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