Chemical effects on the development of the colour-magnitude relation of cluster galaxies
Noelia Jim\'enez, Sof\'ia A. Cora, Lilia P. Bassino, Anal\'ia Smith, Castelli, Tom\'as Tecce

TL;DR
This study uses semi-analytic models and simulations to analyze the development of the colour-magnitude relation in cluster galaxies, confirming its universality and identifying key processes influencing galaxy evolution.
Contribution
It provides a detailed statistical analysis of the processes affecting galaxy properties along the CMR, emphasizing the role of dry mergers in luminous galaxy evolution.
Findings
Good agreement between simulated and observed CMRs.
Dry mergers contribute to galaxy mass growth without changing colours.
The universality of the CMR is supported across different cluster masses.
Abstract
We investigate the development of the colour-magnitude re- lation (CMR) of cluster galaxies. This study is carried out using a semi- analytic model of galaxy formation and evolution coupled to a sample of simulated galaxy clusters of different masses, reinforcing the conclusions reached by Jim\'enez et al. (2009). We compare both simulated and obeserved CMRs in different colour-magnitude planes, finding a very good agreement in all cases. This indicates that model parameters are correctly tuned, giving accurate values of the main properties of galaxies for further use in our study. In the present work, we perform a statistical analysis of the relative contribution to the stellar mass and metallicity of galaxies along the CMR by the different processes involved in their formation and evolution (i.e. quiescent star formation, disc instability events and galaxy mergers). Our results show…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Phase Equilibria and Thermodynamics
