  We present new high resolution and high sensitivity multi-frequency VLA radio
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 position of
the core. The centimetric continuum spectrum of the source is consistent with
thermal emission from ionised gas. This is the first direct evidence that a
newly born massive star is powering the G9.62+0.19-F hot core.
