  The Pierre Auger observatory has presented evidence that the arrival
directions of cosmic rays with energies in excess of 6x10^7 TeV may be
correlated with nearby active galactic nuclei (AGN). In this context we revisit
a suggestion based on gamma ray observations that nearby Fanaroff-Riley I
galaxies such as Cen A and M87 are the sources of the local cosmic rays. We
compute the accompanying neutrino flux and find a flux within reach of
second-generation kilometer-scale neutrino telescopes.
