Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations

Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations

We compare the galaxy population of an SPH simulation to those predicted by the GalICS semi-analytic model and a stripped down version without supernova and AGN feedback. The SPH simulation and the no-feedback GalICS model make similar predictions for the baryonic mass functions of galaxies and for...

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Detalhes bibliográficos
Main Authors: Cattaneo, A, Blaizot, J, Weinberg, D, Colombi, S, Dave, R, Devriendt, J, Guiderdoni, B, Katz, N, Keres, D
Formato: Journal article
Idioma:English
Publicado em: 2006

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