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Paper: Chemical Evolution of the Stellar and Gaseous Components of Galaxies in Hydrodynamical Cosmological Simulations
Volume: 230, Galaxy Disks and Disk Galaxies
Page: 653
Authors: Cora, S. A.; Tissera, P. B.; Lambas, D. G.; Mosconi, M. B.
Abstract: We present preliminary results on the effects of mergers on the chemical properties of galactic objects in hierarchical clustering scenarios. We adopt a hydrodynamical chemical code that allows to describe the coupled evolution of dark matter and baryons within a cosmological context. We found that disk-like and spheroid-like objects have distinctive metallicity patterns that may be the result of different evolution.
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