activity
20242026
collaborators

45 papers

astro-ph.CO2026

Radio Halos in Galaxy Clusters as unveiled by the SKA telescope

R. Cassano, G. Di Gennaro, V. Cuciti +24

Giant radio halos (RHs) are diffuse, Mpc-scale synchrotron sources observed in a growing fraction of galaxy clusters. They trace relativistic particles and magnetic fields in the i…

astro-ph.CO2026

The Large-Scale Structure of the Universe through the SKA lenses

Virginia Cuciti, Surajit Paul, Viral Parekh +11

The large-scale distribution of galaxies in the Universe forms an intricate, interconnected network known as the cosmic web. Cosmological simulations within the standard Lambda-CDM…

astro-ph.CO2026

The Cosmic Ray Life Cycle in Galaxy Clusters

Francesco de Gasperin, Marcus Brüggen, Henrik Edler +3

Within the cosmic web, gravitational energy, linked to the formation and growth of the Universe's largest structures and the activity of active galactic nuclei (AGN), is converted…

astro-ph.GA2026

AGN Jets from Formation to Dissipation

A. -K. Baczko, Eleni Vardoulaki, Etienne Bonnassieux +26

Active Galactic Nuclei (AGN) are among the most energetic phenomena in the Universe, capable of launching powerful relativistic jets that extend from sub-parsec to megaparsec scale…

astro-ph.CO2026

Bulk and turbulent gas motions in the interacting galaxy cluster Abell 3395 South observed with XRISM

Naomi Ota, Angie Veronica, Jakob Dietl +8

We investigate the gas motions in the core region of the Abell~3395 South subcluster (A3395S) using high-resolution X-ray spectroscopy with XRISM/Resolve. By analyzing the Fe~XXV H…

physics.plasm-ph2026

Inverse energy transfer in decaying MHD turbulence: A shell-to-shell analysis

Lenard Kasselmann, Philipp Grete, Pranjal Trivedi +2

In decaying magnetohydrodynamic turbulence, energy can be transported from small to large scales, known as inverse transfer. We explore the mechanism behind this phenomenon using s…