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We have studied the kinematics of the ionized gas and stellar component inMrk334 using methods of panoramic (3D) spectroscopy. The observations wereperformed at the prime focus of the SAO RAS 6-m telescope with theintegral-field spectrograph MPFS (Afanasiev et al. 2001) and with a scanningFabry-Perot interferometer (FPI), installed on the multimode device SCORPIO(Afanasiev & Moiseev 2005). Based on these data, the monochromatic maps andvelocity fields in different emission lines of the ionized gas wereconstructed. The diagnostic diagrams have been made based on the emission linesratios.

Merging as a key to reforming of disk and AGN triggering in Sy galaxy Mrk334