  We study the interaction of early-type stars with the jets of active galactic
nuclei. A bow-shock will form as a consequence of the interaction of the jet
with the winds of stars and particles can be accelerated up to relativistic
energies in these shocks. We compute the non-thermal radiation produced by
relativistic electrons from radio to gamma-rays. This radiation may be
significant, and its detection might yield information on the properties of the
stellar population in the galaxy nucleus, as well as on the relativistic jet.
This emission is expected to be relevant for nearby non-blazar sources.
