We present the kinematical data obtained for a sample of active (Seyfert) and non active isolated spiral galaxies, based on long slit spectra along several position angles in the H{alpha} line region and, in some cases, in the Ca triplet region as well. Gas velocity distributions are presented, together with a simple circular rotation model that allows us to determine the kinematical major axes. Stellar velocity distributions are also shown.
Cone search capability for table J/A+A/416/475/table5 (Emission line measurements for the 224 HII regions for 20 galaxies of our sample having H{alpha} equivalent widths larger than 10{AA})