Merging as a Key to the Reforming of Disk and Active Galactic Nuclei Triggering in Seyfert Galaxy Mrk 334

Details Merging as a Key to the Reforming of Disk and Active Galactic Nuclei Triggering in Seyfert Galaxy Mrk 334 Merging as a Key to the Reforming of Disk and Active Galactic Nuclei Triggering in Seyfert Galaxy Mrk 334

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..396..291s&link_type=abstract

Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at

Astronomy and Astrophysics

Astronomy

Scientific paper

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 tep{mpfs} and with a scanning Fabry-Perot interferometer, installed on the multimode device SCORPIO tep{afan}. 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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