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Environmental Effects on Galaxy Evolution: Multifrequency study of nearby clusters

Published online by Cambridge University Press:  17 August 2016

H. Bravo-Alfaro
Affiliation:
Departamento de Astronomia, Universidad de Guanajuato, Apdo. Postal 144, Mexico. email: hector@astro.ugto.mx Institut d'Astrophysique de Paris, UPMC-CNRS, UMR7095, 98bis Bd Arago, 75014, Paris, France
Y. Venkatapathy
Affiliation:
Departamento de Astronomia, Universidad de Guanajuato, Apdo. Postal 144, Mexico. email: hector@astro.ugto.mx
F. Durret
Affiliation:
Institut d'Astrophysique de Paris, UPMC-CNRS, UMR7095, 98bis Bd Arago, 75014, Paris, France
C. A. Caretta
Affiliation:
Departamento de Astronomia, Universidad de Guanajuato, Apdo. Postal 144, Mexico. email: hector@astro.ugto.mx
V. Gamez
Affiliation:
Departamento de Astronomia, Universidad de Guanajuato, Apdo. Postal 144, Mexico. email: hector@astro.ugto.mx
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Abstract

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We show first results of a multifrequency survey focused on the mechanisms driving the transformation of cluster galaxies, from late to earlier S0-types. We compare the ram-pressure effects seen on 21cm-HI images with those mechanisms affecting the old stellar disks seen on deep optical and NIR images. Our targets are the Abell clusters A85, A496, A2670, which span different relaxation degrees, masses and X-ray luminosities.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016