We present new high resolution and high sensitivity multi-frequency VLA rad
io continuum observations of the G9.62+0.19-F hot molecular core. We detect
for the first time faint centimetric radio continuum emission at the posit
ion of the core. The centimetric continuum spectrum of the source is consis
tent with thermal emission from ionised gas. This is the first direct evide
nce that a newly born massive star is powering the G9.62+0.19-F hot core.