We have conducted a 3.6 cm radio-continuum survey with the VLA in its compa
ct D-array to look for extended radio-continuum emission around known ultra
compact H II regions. We find extended emission in 12 out of 15 fields. The
extended emission ranges in size up to 5', with typical diameters of 60 ",
or 2 pc. In some cases, the extended component produces an order of magnit
ude more flux than the ultracompact component. It is possible that the exte
nded emission is from H II regions not connected with the ultracompact H II
regions, but on the basis of the morphology of the emission, we believe th
at it is possible or even likely that the ultracompact and extended emissio
n are directly connected in about half of the sources. The possible consequ
ences of directly connected extended emission are profound. We may be force
d to reconsider the definition of an ultracompact H rr region and consider
models in which dense, ultracompact ionized components are embedded in less
dense, more extended regions.