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20242026
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astro-ph.CO2024

The ViCTORIA project: description of a multi-frequency radio survey of the Virgo galaxy cluster

F. de Gasperin, H. W. Edler, A. Boselli +8

The Virgo cluster is the closest richest nearby galaxy cluster. It is in the formation process, with a number of sub-clusters undergoing merging and interactions. Although a great…

astro-ph.GA2024

Euclid: Early Release Observations -- The intracluster light and intracluster globular clusters of the Perseus cluster

M. Kluge, N. A. Hatch, M. Montes +185

We study the intracluster light (ICL) and intracluster globular clusters (ICGCs) in the nearby Perseus galaxy cluster using Euclid's EROs. By modelling the isophotal and iso-densit…

astro-ph.GA2024

A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE): XVI. The ubiquity of truncated star-forming disks across the Virgo cluster environment

C. R. Morgan, M. L. Balogh, A. Boselli +14

We examine the prevalence of truncated star-forming disks in the Virgo cluster down to . This work makes use of deep, high-resolution imaging in…

astro-ph.HE2024

ViCTORIA project: The LOFAR-MeerKAT view of AGN in Virgo cluster early-type galaxies

A. Spasic, H. W. Edler, Y. Su +8

The evolution of Active Galactic Nuclei (AGN) is closely connected to their host galaxies and surroundings. Via feedback processes, AGN can counteract the cooling of the intraclust…

astro-ph.GA2024

Euclid: Early Release Observations -- Dwarf galaxies in the Perseus galaxy cluster

F. R. Marleau, J. -C. Cuillandre, M. Cantiello +193

We make use of the unprecedented depth, spatial resolution, and field of view of the Euclid Early Release Observations of the Perseus galaxy cluster to detect and characterise the…

astro-ph.GA2024

Euclid: Early Release Observations -- Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions

J. -C. Cuillandre, M. Bolzonella, A. Boselli +199

The Euclid ERO programme targeted the Perseus cluster of galaxies, gathering deep data in the central region of the cluster over 0.7 square degree, corresponding to approximately 0…