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

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.

preprint2020arXivOpen access
L. J. ZenocrattiA. V. Smith CastelliM. E. De RossiF. R. Faifer
astro-ph.GA
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Open access4 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
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L. J. ZenocrattiA. V. Smith CastelliM. E. De RossiF. R. Faifer

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