Stellar populations in (U)LIRGs and post-starburst QSOs

Details Stellar populations in (U)LIRGs and post-starburst QSOs Stellar populations in (U)LIRGs and post-starburst QSOs

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sacm.confe..38c&link_type=abstract

The Starburst-AGN Connection under the Multiwavelength Limelight, held 14-16 September 2011. Published online at http://www.scio

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Scientific paper

Within the hierarchical model, it is believed that galactic mergers (like those happening in Ultraluminous Infrared Galaxies, ULIRGs) could generate starburst processes (SBs) that would feed a central AGN. The final stage, once the gas has been dissipated, is the formation of elliptical galaxies. In other words, we want to investigate the evolutionary sequence: (U)LIRGs -> POST-SBs -> QSOs -> ellipticals. For doing so we are are studying the stellar populations (SPs) in two samples of (U)LIRGs and POST-SBs QSOs galaxies for which we have optical integral field spectroscopy (IFS-PMAS@CAHA) data and HST high resolution multiwavelength imaging (from NUV to NIR). Using the ages of the SPs as a clock we can check whether or not an evolutionary link exists between them. In this poster we present the first results of the analysis of these data.

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