  We have used the Australia Telescope Compact Array (ATCA) to search for
continuum emission toward three strong 6.7-GHz methanol maser sources. For two
of the sources, G339.88-1.26 and NGC 6334F (G351.42+0.64), we detect continuum
emission closely associated with the methanol masers. A further three clusters
of masers showed no radio continuum emission above our sensitivity limit of 1-5
mJy. We find the position of the 6.7-GHz methanol masers in G339.88-1.26 to be
consistent with the hypothesis that the masers lie in the circumstellar disc
surrounding a massive star. We also argue that one of the clusters of methanol
masers in NGC 6334F provides indirect observational support for the
circumstellar disc hypothesis.
