A substantial body of evidence now exists that indicates that there is
a connection between the observed activity in galaxies and the appare
nt involvement of these active galaxies in tidal interactions with oth
er galaxies. To investigate this phenomenon, we are studying the morph
ologies and environments of various interacting galaxies showing evide
nce of activity. In particular, we present here some preliminary resul
ts from our investigations of the claimed interaction-activity connect
ion for a sample of colliding radio galaxies endowed with a bent radio
jet morphology. We find that the timing of the jet activity is consis
tent with a tidal-triggering hypothesis. Our results therefore lend fu
rther support to the idea that the galactic activity observed in some
''interactive'' galaxies is in fact collision-induced.