  We present observations between 14.2 and 17.9 GHz of sixteen Galactic HII
regions made with the Arcminute Microkelvin Imager (AMI). In conjunction with
data from the literature at lower radio frequencies we investigate the
possibility of a spinning dust component in the spectra of these objects. We
conclude that there is no significant evidence for spinning dust towards these
sources and measure an average spectral index of 0.15+/-0.07 between 1.4 and
17.9 GHz for the sample.
