  We present observations of the Cygnus OB2 region obtained with the Giant
Metrewave Radio Telescope (GMRT) at the frequencies of 325 MHz and 610 MHz. In
this contribution we focus on the study of proplyd-like objects (also known as
free-floating Evaporating Gas Globules or frEGGs) that typically show an
extended cometary morphology. We identify eight objects previously studied at
other wavelengths and derive their physical properties by obtaining their
optical depth at radio-wavelengths. Using their geometry and the
photoionization rate needed to produce their radio-continuum emission, we find
that these sources are possibly ionized by a contribution of the stars Cyg OB2
#9 and Cyg OB2 #22. Spectral index maps of the eight frEGGs were constructed,
showing a flat spectrum in radio frequencies in general. We interpret these as
produced by optically-thin ionized gas, although it is possible that a
combination of thermal emission, not necessarily optically thin, produced by a
diffuse gas component and the instrument response (which detects more diffuse
emission at low frequencies) can artificially generate negative spectral
indices. In particular, for the case of the Tadpole we suggest that the
observed emission is not of non-thermal origin despite the presence of regions
with negative spectral indices in our maps.
