activity
20172022
most citedProperties of galaxies with ring structures

15 citations · 85 across the 8 of their papers we have counts for

collaborators

12 papers

astro-ph.GA20229 cited

A deep near-infrared view of the Ophiuchus galaxy cluster

D. Galdeano, G. Coldwell, F. Duplancic +8

Context: The Ophiuchus cluster of galaxies, located at low latitudes in the direction of the Galactic bulge, has been relatively poorly studied in comparison with other rich galaxy…

astro-ph.GA202115 cited

Properties of galaxies with ring structures

Julia Fernandez, Sol Alonso, Valeria Mesa +2

Aims: We present a statistical analysis of different characteristics of ringed spiral galaxies with the aim of assessing the effects of rings on disk galaxy properties. Methods: We…

astro-ph.GA202111 cited

AGNs in Small Galaxy Systems: comparing the main properties of active objects in pairs, triplets and groups

Fernanda Duplancic, Diego G. Lambas, Sol Alonso +1

We perform a comparative study of AGNs in pairs, triplets and groups. To this end we use the Duplancic et al. catalogue of small galaxy systems and consider BPT and WHAN diagnostic…

astro-ph.GA202110 cited

Overdensity of VVV galaxies behind the Galactic bulge

Daniela Galdeano, Luis Pereyra, Fernanda Duplancic +7

We studied a region of 1.636 square degrees corresponding to the VVV tile . Using SExtractor, we analysed photometric data generating a catalogue of extended sources in this…

astro-ph.GA20204 cited

Satellites and central galaxies in SDSS: the influence of interactions on their properties

Valeria Mesa, Sol Alonso, Georgina Coldwell +2

We use SDSS-DR14 to construct a sample of galaxy systems consisting of a central object and two satellites. We adopt projected distance and radial velocity difference criteria and…

astro-ph.GA202014 cited

The Global Environment of Small Galaxy Systems

Fernanda Duplancic, Federico Dávila-Kurbán, Georgina V. Coldwell +2

The main goal of this work is to investigate the influence of environment at different scales on the properties of galaxies in systems with a low number of members. To this end we…