Chemical and morphological analysis of simulated galaxies

Details Chemical and morphological analysis of simulated galaxies Chemical and morphological analysis of simulated galaxies

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..128p&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Mathematics

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Cosmology: Theory, Galaxies: Evolution, Galaxies: Formation

Scientific paper

We present preliminary results of a study of the abundance and age gradients of disc and spheroid components in galaxies selected from hydrodynamical cosmological simulations consistent with the concordance Λ-CDM models. Our simulated abundance and age gradients are in agreement with observations at z = 0. Abundance gradients for disc components are found to be steeper at higher redshifts.

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