248 citations · 1.8k across the 97 of their papers we have counts for
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Galaxy cluster mergers as triggers for the formation of jellyfish galaxies: case study of the A901/2 system
Rafael Ruggiero, Rubens E. G. Machado, Fernanda V. Roman-Oliveira +4
The A901/2 system is a rare case of galaxy cluster interaction, in which two galaxy clusters and two smaller groups are seen in route of collision with each other simultaneously. W…
OMEGA -- OSIRIS Mapping of Emission-line Galaxies in A901/2 -- V. The rich population of jellyfish galaxies in the multi-cluster system Abell 901/2
Fernanda V. Roman-Oliveira, Ana L. Chies-Santos, Bruno Rodríguez del Pino +3
We present the results of a systematic search and characterisation of jellyfish galaxy candidates in the multi-cluster system A901/2, at z ~ 0.165, as part of the OMEGA survey. By…
J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX
D. D. Whitten, V. M. Placco, T. C. Beers +24
We present a new methodology for the estimation of stellar atmospheric parameters from narrow- and intermediate-band photometry of the Javalambre Photometric Local Universe Survey…
J-PLUS: analysis of the intracluster light in the Coma cluster
Y. Jiménez-Teja, R. A. Dupke, R. Lopes de Oliveira +19
The intracluster light (ICL) is a luminous component of galaxy clusters composed of stars that are gravitationally bound to the cluster potential but do not belong to the individua…
OMEGA - OSIRIS Mapping of Emission-line Galaxies in A901/2: IV. - Extinction of Star-Formation Estimators with Inclination
Christian Wolf, Tim Weinzirl, Alfonso Aragón-Salamanca +6
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral passbands that are commonly used as star-formation indicators. As diagnostics we…
Chromodynamical Analysis of Lenticular Galaxies using Globular Clusters and Planetary Nebulae
Emilio J. B. Zanatta, Arianna Cortesi, Ana L. Chies-Santos +7
Recovering the origins of lenticular galaxies can shed light on the understanding of galaxy formation and evolution, since they present properties that can be found in both ellipti…