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The Planck 28.5 GHz maps were searched for potential Anomalous MicrowaveEmission (AME) regions on the scale of $\sim3^{\circ}$ or smaller, and severalnew regions of interest were selected. Ancillary data at both lower and higherfrequencies were used to construct spectral energy distributions (SEDs), whichseem to confirm an excess consistent with spinning dust models. Here we presenthigher resolution observations of two of these new regions with the ArcminuteMicrokelvin Imager Small Array (AMI SA) between 14 and 18 GHz to test for thepresence of a compact ($\sim$10 arcmin or smaller) component. ForAME-G107.1+5.2, dominated by the {\sc Hii} region S140, we find evidence forthe characteristic rising spectrum associated with the either the spinning dustmechanism for AME or an ultra/hyper-compact \textsc{Hii} region across the AMIfrequency band, however for AME-G173.6+2.8 we find no evidence for AME onscales of $\sim 2-10$ arcmin.

Investigating the source of Planck-detected AME: high resolution observations at 15 GHz