Upload resources

Upload your works to SEDICI to increase its visibility and improve its impact

 

Development of the red sequence in galaxy clusters

Document type: Comunicacion

Abstract

We investigate the origin of the color-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 defined by less luminous galaxies could be explained by the influence of minor mergers.

General information

Issue date: 2009
Document language: English
Journal: Proceedings of the International Astronomical Union; vol. 5, no. S267
Event: IAU Symposium 267 (Rio de Janeiro, Brazil, 2009)
Origin: Instituto de Astrofísica de La Plata; Facultad de Ciencias Astronómicas y Geofísicas
Others identifiers: eid:2-s2.0-84884950605
ISSN: 1743-9213
Pages: 460-460
xmlui.dri2xhtml.METS-1.0.item-dc-subject: Galaxies: clusters ; Galaxies: evolution
Subjects: Ciencias Astronómicas

Download Files

Thumbnail
Documento completo
Download file (189.3Kb) - PDF
 
Created: 4 de octubre de 2019
Available since: 4 de octubre de 2019
Please, use one of this identificators(URI) for cite o linking this item:
  • http://sedici.unlp.edu.ar/handle/10915/82789
  • https://doi.org/10.1017/S1743921310007027

    • This item appears in the following Collection(s)

    Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)