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Abstract

We aim to use N-body simulations in order to investigate how dissipation-less merging affects internal color gradients and structural properties of early-type galaxies. Galaxies are modeled as spherical, two-components, non-rotating systems. The dark matt

Item Type: Conference or Workshop Item (UNSPECIFIED)
Depositing User: ing Paolo Nicastro
Date Deposited: 18 Oct 2010 08:15
Last Modified: 30 Apr 2014 19:41
URI: http://www.fedoa.unina.it/id/eprint/5580

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