  The IceCube experiment has recently reported the first observation of
high-energy cosmic neutrinos. Their origin is still unknown. In this paper, we
investigate the possibility that they originate in active galaxies. We show
that hadronic interactions (pp) in the generally less powerful, more frequent,
FR-I radio galaxies are one of the candidate source classes being able to
accommodate the observation while the more powerful, less frequent, class of
FR-II radio galaxies has too low of a column depths to explain the signal.
