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20052023
most citedGalaxy populations in the Antlia cluster. I. Photometric properties of early-type galaxies

58 citations · 261 across the 24 of their papers we have counts for

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Showing 2011Show all

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astro-ph.CO2011★ 24 cited

Galaxy populations in the Antlia cluster - III. Properties of faint early-type galaxies

Analia V. Smith Castelli, Sergio A. Cellone, Favio R. Faifer +5

(Abridge) We present a new analysis of the early-type galaxy population in the central region of the Antlia cluster, focusing on the faint systems like dwarf ellipticals (dE) and d…

astro-ph.CO2011★ 1 cited

Development of the Red Sequence in Galaxy Clusters

Noelia Jiménez, Sofía A. Cora, Analía Smith Castelli +1

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…

astro-ph.CO2011★ 34 cited

The bright end of the colour-magnitude relation of cluster galaxies

Noelia Jiménez, Sofía A. Cora, Lilia P. Bassino +2

We investigate the development of the red sequence (RS) of cluster galaxies by using a semi-analytic model of galaxy formation. Results show good agreement between the general tren…

astro-ph.GA2011

Chemical effects on the development of the colour-magnitude relation of cluster galaxies

Noelia Jiménez, Sofía A. Cora, Lilia P. Bassino +2

We investigate the development of the colour-magnitude re- lation (CMR) of cluster galaxies. This study is carried out using a semi- analytic model of galaxy formation and evolutio…

astro-ph.CO2011

Modeling the Color Magnitude Relation for Galaxy Clusters

Noelia Jimenez, Sofia A. Cora, Analia Smith Castelli +1

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 an…

astro-ph.GA2011

The Color-Magnitude Relation of Cluster Galaxies: Observations and Model Predictions

Noelia Jimenez, Analia Smith Castelli, Sofia A. Cora +1

We investigate the origin of the color-magnitude relation (CMR) observed in cluster galaxies by using a combination of cosmological N-body/SPH simulations of galaxy clusters, and a…