Artículo

Modeling the color magnitude relation for galaxy clusters

Jiménez, NoeliaIcon ; Cora, Sofia AlejandraIcon ; Smith Castelli, Analia VivianaIcon ; Bassino, Lilia PatriciaIcon
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
 
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Licencia
info:eu-repo/semantics/openAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)
Identificadores
URI: http://hdl.handle.net/11336/9430
URL: http://www.aspbooks.org/a/volumes/article_details/?paper_id=31728
URL: https://arxiv.org/abs/1106.3337
Colecciones
Articulos(IALP)
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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