activity
20162024
most citedSimulations of extragalactic magnetic fields and of their observables

129 citations · 505 across the 18 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA20239 cited

Unraveling Baroclinicity in Black Hole Weather Storms

Denis Wittor, Massimo Gaspari

In the intracluster, intragroup, and circumgalactic medium (ICM, IGrM, CGM), turbulence plays a vital role in the self-regulated feedback and feeding cycle of central supermassive…

astro-ph.GA2021

Bent it like FRs: extended radio AGN in the COSMOS field and their large-scale environment

Eleni Vardoulaki, Franco Vazza, Eric F. Jiménez-Andrade +3

One of the fascinating topics in radio astronomy is how to associate the complexity of observed radio structures to their environment, in order to understand their interplay and th…

astro-ph.GA202049 cited

Physical insights from the spectrum of the radio halo in MACS J0717.5+3745

K. Rajpurohit, G. Brunetti, A. Bonafede +18

We present new LOFAR observations of the massive merging galaxy cluster MACS J0717.5+3745. The cluster hosts the most powerful radio halo known to date. These new observations, in…

astro-ph.GA202036 cited

Understanding the radio relic emission in the galaxy cluster MACS J0717.5+3745: spectral analysis

K. Rajpurohit, D. Wittor, R. J. van Weeren +21

Radio relics are diffuse, extended synchrotron sources that originate from shock fronts generated during cluster mergers. The massive merging galaxy cluster MACS J0717.5+3745 hosts…

astro-ph.GA2020

Dissecting the turbulent weather driven by mechanical AGN feedback

D. Wittor, M. Gaspari

Turbulence in the intracluster, intragroup, and circumgalactic medium plays a crucial role in the self-regulated feeding and feedback loop of central supermassive black holes. We d…

astro-ph.GA202022 cited

Spectro-polarimetric observations of the CIZA J2242.8+5301 northern radio relic: no evidence of high-frequency steepening

Francesca Loi, Matteo Murgia, Valentina Vacca +16

Observations of radio relics at very high frequency (>10 GHz) can help to understand how particles age and are (re-)accelerated in galaxy cluster outskirts and how magnetic fields…