  We present radio continuum images of three Galactic HII regions, S 201, S
206, and S 209 near 232, 327, and 610 MHz using the Giant Meterwave Radio
Telescope (GMRT). The GMRT has a mix of short and long baselines, therefore,
even though the data have high spatial resolution, the maps are still sensitive
to diffuse extended emission. We find that all three HII regions have bright
cores surrounded by diffuse envelopes. We use the high resolution afforded by
the data to estimate the electron temperatures and emission measures of the
compact cores of these HII regions. Our estimates of electron temperatures are
consistent with a linear increase of electron temperature with Galacto-centric
distance for distances up to 18 kpc (the distance to the most distant HII
region in our sample).
