  In order to quantify the relationship between gas accretion and star
formation, we analyse a sample of 29 nearby galaxies from the WHISP survey
which contains galaxies with and without evidence for recent gas accretion. We
compare combined radial profiles of FUV (GALEX) and IR 24 {\mu}m (Spitzer)
characterizing distributions of recent star formation with radial profiles of
CO (IRAM, BIMA, or CARMA) and HI (WSRT) tracing molecular and atomic gas
contents to examine star formation efficiencies in symmetric (quiescent),
asymmetric (accreting), and interacting (tidally disturbed) galaxies. In
addition, we investigate the relationship between star formation rate and HI in
the outer discs for the three groups of galaxies. We confirm the general
relationship between gas surface density and star formation surface density,
but do not find a significant difference between the three groups of galaxies.
