VEGAS: A VST Early-type GAlaxy Survey. III. Mapping the galaxy structure, interactions and intragroup light in the NGC 5018 group
Marilena Spavone, Enrichetta Iodice, Massimo Capaccioli, Daniela, Bettoni, Roberto Rampazzo, Noah Brosch, Michele Cantiello, Nicola R., Napolitano, Luca Limatola, Aniello Grado, Pietro Schipani

TL;DR
This study presents deep multiband imaging of the NGC 5018 galaxy group, revealing extensive intragroup light, interactions among members, and insights into galaxy evolution within groups.
Contribution
It provides the first detailed mapping of the galaxy structure, interactions, and intragroup light in the NGC 5018 group using deep VST imaging.
Findings
41% of group luminosity is intragroup light.
Detected tidal tails and ring-like structures indicating ongoing interactions.
Evidence of a minor merger affecting NGC 5018's structure.
Abstract
Most of the galaxies in the Universe at present day are in groups, which are key to understanding the galaxy evolution. In this work we present a new deep mosaic of 1.2 x 1.0 square degrees of the group of galaxies centered on NGC 5018, acquired at the ESO VLT Survey Telescope. We use u, g, r images to analyse the structure of the group members and to estimate the intra-group light. Taking advantage of the deep and multiband photometry and of the large field of view of the VST telescope, we studied the structure of the galaxy members and the faint features into the intra-group space and we give an estimate of the intragroup diffuse light in the NGC 5018 group of galaxies. We found that ~ 41% of the total g-band luminosity of the group is in the form of intragroup light (IGL). The IGL has a (g - r) color consistent with those of other galaxies in the group, indicating that the stripping…
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