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      Evolution of the colour-magnitude relation of early-type galaxies in cosmological numerical simulations

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          Abstract

          In this work, we study the evolution with redshift of the colour-magnitude relation (CMR) of early-type galaxies. This evolution is analyzed through cosmological numerical simulations from z = 2 to z = 0. The preliminary results shown here represent the starting point of a study aimed at identifying the processes that originated the observed CMR of early-type galaxies at z = 0.

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          Author and article information

          Journal
          10 May 2020
          Article
          2005.04716

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          Custom metadata
          3 pages, 2 figures. Accepted for publication in BAAA V61B
          astro-ph.GA

          Galaxy astrophysics

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