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Evolutionary status of galaxy population in clusters at intermediate redshift (z ~ 0.2)

Published online by Cambridge University Press:  07 August 2017

Emilio Molinari ,
Dolores Pedrana ,
Massimo Banzi ,
Alberto Buzzoni  and
Guido Chincarini
Emilio Molinari
Affiliation:
Osservatorio Astronomico di Brera Via Brera, 28 20121 Milano, Italy
Dolores Pedrana
Affiliation:
Osservatorio Astronomico di Brera Via Brera, 28 20121 Milano, Italy
Massimo Banzi
Affiliation:
Osservatorio Astronomico di Brera Via Brera, 28 20121 Milano, Italy
Alberto Buzzoni
Affiliation:
Osservatorio Astronomico di Brera Via Brera, 28 20121 Milano, Italy
Guido Chincarini
Affiliation:
Osservatorio Astronomico di Brera Via Brera, 28 20121 Milano, Italy

Extract

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In this contribution we present observations for a set of three clusters of galaxies at intermediate redshift (z ~ 0.2) selected from the revised Abell catalog (Abell et al. 1989, Ap.J. Suppl., 70, 1) and observed in the Gunn photometric system at the ESO 3.6m telescope in La Silla (Chile) during various runs between 1986 and 1990. This is part of a more extended project addressing the study of the distant clusters, as outlined in more detail in Molinari et al. (1990, M.N.R.A.S., 246, 576).

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 460
Copyright
Copyright © Kluwer