We have studied two galaxies with active nuclei using the methods of panoramic spectroscopy. In order to investigate the kinematics of ionized gas and stars, we carried out observations at 6-m telescope of the SAO RAS with the integral field spectrograph MPFS. We have created intensity maps and velocity fields in different emission lines of the ionized gas as well as velocity fields for the stellar component. Diagnostic diagrams have also been made based on the emission lines ratios. © 2007 Springer-Verlag Berlin Heidelberg.
CITATION STYLE
Smirnova, A. A., Moiseev, A. V., & Afanasiev, V. L. (2007). Studying of some seyfert galaxies by means of panoramic spectroscopy. In ESO Astrophysics Symposia (Vol. 2007, pp. 285–287). https://doi.org/10.1007/978-3-540-73491-8_47
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