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Environmental Effects on Galaxy Luminosity Functions in Clusters

Published online by Cambridge University Press:  05 December 2011

Florence Durret ,
Christophe Adami  and
Tatiana F. Laganá
Florence Durret
Affiliation:
UPMC Université Paris 06, UMR 7095, Institut d'Astrophysique de Paris, 98bis Bd Arago, F-75014, Paris, France, email: durret@iap.fr CNRS, UMR 7095, Institut d'Astrophysique de Paris, F-75014 Paris, France
Christophe Adami
Affiliation:
LAM, Pôle de l'Etoile Site de Château-Gombert, 38 rue Frédéric Joliot-Curie, 13388 Marseille Cedex 13, France
Tatiana F. Laganá
Affiliation:
IAG, USP, R. do Matão 1226, 05508-090, São Paulo/SP, Brazil
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Abstract

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The formation and evolution of galaxies is strongly influenced by environment, particularly in clusters, where galaxy luminosity functions vary in shape with the dynamical state of the cluster (relaxed or in various stages of merging), with the photometric band considered and with the position in the cluster. We present here results concerning the optical GLFs in several relaxed and merging clusters.

Keywords

galaxies: clusters: individual (Coma, A85, A222/223, A496, A780, A1758), galaxies: luminosity function
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S277: Tracing the Ancestry of Galaxies (on the land of our ancestors) , December 2010 , pp. 9 - 12
Copyright
Copyright © International Astronomical Union 2011

References

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