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Paper: Merging as a Key to the Reforming of Disk and Active Galactic Nuclei Triggering in Seyfert Galaxy Mrk 334
Volume: 396, Formation and Evolution of Galaxy Disks
Page: 291
Authors: Smirnova, A.; Moiseev, A.V.
Abstract: We have studied the kinematics of the ionized gas and stellar component in Mrk 334 using methods of panoramic (3D) spectroscopy. The observations were performed at the prime focus of the SAO RAS 6-m telescope with the integral-field spectrograph Multi-Pupil Fiber Spectrograph (Afanasiev et al. 2001) and with a scanning Fabry-Perot interferometer, installed on the multimode device SCORPIO (Afanasiev & Moiseev 2005). Based on these data, the monochromatic maps and velocity fields in different emission lines of the ionized gas were constructed. The diagnostic diagrams have been made based on the emission lines ratios.
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