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Paper: Probing the Stellar Populations of Early-Type Galaxies: the SAURON Survey (Invited Talk)
Volume: 282, Galaxies: The Third Dimension
Page: 189
Authors: Emsellem, E.; Davies, R.; McDermid, R.; Kuntschner, H.; Peletier, R.; Bacon, R.; Bureau, M.; Cappellari, M.; Copin, Y.; Miller, B.; Verolme, E.; de Zeeuw, T.
Abstract: Studying the role and dynamics of nuclear density waves, in the form of bars, spirals or lopsided density distributions requires the two-dimensional mapping of their kinematics. I will present evidences for the presence of such structures using new sets of observations, and particularly OASIS integral field spectrography. I will thus emphasize the importance of nuclear m=1 modes, illustrating this with newly revealed cases and original N body simulations. I will then discuss the implications of these results in the context of AGN, starburst and dynamical evolution.
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