Artículo
Modeling the color magnitude relation for galaxy clusters
Fecha de publicación:
10/2010
Editorial:
University Of Chicago Press
Revista:
Publications Of The Astronomical Society Of The Pacific
ISSN:
0004-6280
ISBN:
9781583817230
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
We investigate the origin of the colour-magnitude relation (CMR) observed
in cluster galaxies by using a combination of a cosmological N-body simulation
of a cluster of galaxies and a semi-analytic model of galaxy formation. The
departure of galaxies in the bright end of the CMR with respect to the trend
denoted by less luminous galaxies could be explained by the influence of minor
mergers.
Palabras clave:
Galaxies
,
Clusters
,
Models
Archivos asociados
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Identificadores
Colecciones
Articulos(IALP)
Articulos de INST.DE ASTROFISICA LA PLATA
Articulos de INST.DE ASTROFISICA LA PLATA
Citación
Jiménez, Noelia; Cora, Sofia Alejandra; Smith Castelli, Analia Viviana; Bassino, Lilia Patricia; Modeling the color magnitude relation for galaxy clusters; University Of Chicago Press; Publications Of The Astronomical Society Of The Pacific; 421; 10-2010; 261-261
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