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Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations
Authors:Andrea Cattaneo,Jé    my Blaizot,David H. Weinberg,Dusan Kere&#  ,Sté  phane Colombi,Romeel Davé  ,Julien Devriendt,Bruno Guiderdoni, Neal Katz
Affiliation:Astrophysikalisches Institut Potsdam, an der Sternwarte 16, 14482 Potsdam, Germany;Institut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014 Paris, France;Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str.1, 85740 Garching, Germany;Ohio State University, Department of Astronomy, Columbus, OH 43210, USA;Astronomy Department, University of Massachusetts at Amherst, MA 01003, USA;University of Arizona, Steward Observatory, Tucson, AZ 85721, USA;Centre de Recherche Astronomique de Lyon, 9 Avenue Charles André, 69561, St-Genis-Laval Cedex, France
Abstract:
Keywords:cooling flows    galaxies: evolution    galaxies: formation    galaxies: haloes    galaxies: ISM
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