Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008an....329..908d&link_type=abstract
Astronomische Nachrichten, Vol.329, Issue , p.908
Astronomy and Astrophysics
Astronomy
Galaxies: Active, Galaxies: Kinematics And Dynamics, Galaxies: Seyfert, Ism: Kinematics And Dynamics, Stars: Kinematics
Scientific paper
We investigate the kinematic properties of the stars and ionised gas in the circumnuclear regions of a matched sample of nearby Seyfert and non-active galaxies, using the SAURON Integral-Field Unit (IFU) on the William Herschel Telescope (WHT). In both active and non-active galaxies, the stellar velocity fields present regular rotation patterns. After removal of the non-gravitational components due to nuclear activity (e.g., AGN-driven outflows) in the case of the Seyfert galaxies, the ionised gas kinematics in both populations is dominated by rotation. The non-active galaxies present a global alignment between stellar and gaseous kinematics while majority of Seyfert galaxies present strong kinematics misalignments between the two components. A more refined analysis of our two-dimensional kinematics maps reveal evidence for deviations from axial-symmetry in the gaseous velocity fields. These deviations are moreover stronger in the case of Seyfert galaxies than their associated non-active galaxies. This result suggests the presence of weak dynamical perturbations in the circumnuclear regions of Seyfert galaxies and provides a tentative link between nuclear activity and the host galaxy dynamics in these regions.
Dumas Gaelle
Emsellem Eric
Mundell Carole G.
Nagar Neil
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