Nature versus nurture: relic nature and environment of the most massive passive galaxies at $z < 0.5$
C. Tortora, N. R. Napolitano, M. Radovich, C. Spiniello, L. Hunt, N., Roy, L. Moscardini, D. Scognamiglio, M. Spavone, M. Brescia, S. Cavuoti, G., D`Ago, G. Longo, F. Bellagamba, M. Maturi, M. Roncarelli

TL;DR
This study investigates the distribution of ultracompact massive galaxies, likely relics of early galaxy formation, across different environments, revealing that their abundance is only mildly affected by environment, suggesting stochastic merging processes dominate their survival.
Contribution
It provides observational evidence that relic galaxy abundance depends more on stochastic merging history than on environmental density.
Findings
UCMGs are more common in clusters but not exclusively.
Relic galaxies' survival is only mildly influenced by environment.
Merging stochasticity plays a key role in relics' presence.
Abstract
Relic galaxies are thought to be the progenitors of high-redshift red nuggets that for some reason missed the channels of size growth and evolved passively and undisturbed since the first star formation burst (at ). These local ultracompact old galaxies are unique laboratories for studying the star formation processes at high redshift and thus the early stage of galaxy formation scenarios. Counterintuitively, theoretical and observational studies indicate that relics are more common in denser environments, where merging events predominate. To verify this scenario, we compared the number counts of a sample of ultracompact massive galaxies (UCMGs) selected within the third data release of the Kilo Degree Survey, that is, systems with sizes and stellar masses , with the number counts of galaxies with the…
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