We have used photometric images of ten barred galaxies in the B and I bands
to infer the geometrical and dynamical parameters of their bars: Their len
gth, (R-bar), their strengths, (S-b), and their corotation radii, (R-CR). T
hese parameters have been obtained studying azimuthal profiles from the B a
nd I band images of the galaxies. We find that R-CR is in all cases slightl
y larger than R-bar, with mean values close to 1.2 R-bar. We have also foun
d a dependence of the ratio R-CR/R-bar on S-bar.