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- W3040901826 abstract "We investigate the origin of the color-magnitude relation (CMR) observed in cluster galaxies by using a combination of cosmological N-body/SPH simulations of galaxy clusters, and a semi-analaytic model of galaxy formation (Lagos, Cora & Padilla 2008). Simulated results are compared with the photometric properties of early-type galaxies in the Antlia cluster (Smith Castelli et al. 2008). The good agreement obtained between observations and simulations allows us to use the information provided by the model for unveiling the physical processes that yield the tigh observed CMR. Resumen. Investigamos la relacion color-magnitud (CMR) observada en cumulos de galaxias, usando simulaciones hidrodinamicas cosmologicas de N-cuerpos de cumulos de galaxias junto con un modelo semianaĺitico de formacion de galaxias (Lagos, Cora & Padilla 2008). Los resultados de las simulaciones son comparados con las propiedades fotometricas de galaxias de tipo temprano del cumulo de Antlia (Smith Castelli et al. 2008). El buen acuerdo obtenido entre las observaciones y los resultados del modelo, nos permiten utilizar la informacion suministrada por este en el estudio de los procesos fisicos que conducen a una CMR observada muy bien definida." @default.
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- W3040901826 date "2008-01-01" @default.
- W3040901826 modified "2023-09-24" @default.
- W3040901826 title "The Color-Magnitude Relation of Cluster Galaxies: Observations and Model Predictions" @default.
- W3040901826 hasPublicationYear "2008" @default.
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