Аннотация:The results of kinematic investigation of ionized gas in the central parts of Seyfert galaxies with large bars Mrk 79 and Mrk 1126 obtained with the 6-m telescope are presented. The peculiarities of the velocity fields (the turn of the kinematic major axis, the increase of angular rotation velocity with the distance from the center) give evidences of the non-axisymmetrical potential form in the centers of the galaxies being non-similar to their large bars. There are some proofs of radial gas flows with the velocities to ≅200 km/s.