activity
20032026
most citedConstraining the population of cosmic ray protons in cooling flow clusters with gamma-ray and radio observations: Are radio mini-halos of hadronic origin?

282 citations · 9.3k across the 182 of their papers we have counts for

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55 papers · 1 filter

astro-ph.HE2026

Zooming in on radio relics -- II. How relic morphology probes density fluctuations at the edge of galaxy clusters

Joseph Whittingham, Christoph Pfrommer, Maria Werhahn +2

Gas properties in the outer intracluster medium (ICM) are not well-constrained, as traditional probes lose sensitivity at Mpc distances. We show that the morphology of radio relics…

astro-ph.HE2026

Identifying heating processes in simulations with an entropy-based scheme: A single jet episode in a galaxy cluster

Moun Meenakshi, Rainer Weinberger, Christoph Pfrommer +1

Understanding heating processes in galaxy clusters is essential for predicting the regulation of radiative cooling and star formation, and for clarifying the mechanisms underlying…

astro-ph.HE2026

The diffuse gamma-ray sky of a Milky Way analogue: Local diversity and global constraints

Karin Kjellgren, Philipp Girichidis, Maria Werhahn +8

Diffuse gamma-ray emission is a key tracer of cosmic rays (CRs) in galaxies, encoding information about their transport, energetics, and interactions with the interstellar medium.…

astro-ph.HE2025

Disentangling AGN Feedback and Sloshing in the Perseus Cluster with XRISM: Insights from Simulations

Elena Bellomi, John A. ZuHone, Nhut Truong +10

High-resolution X-ray spectroscopy with XRISM has revealed complex, non-monotonic velocity dispersion profiles in the Perseus cluster, pointing to a complex interplay between at le…

astro-ph.HE2024★ 4 cited

Zooming-in on cluster radio relics -- I. How density fluctuations explain the Mach number discrepancy, microgauss magnetic fields, and spectral index variations

Joseph Whittingham, Christoph Pfrommer, Maria Werhahn +2

It is generally accepted that radio relics are the result of synchrotron emission from shock-accelerated electrons. Current models, however, are still unable to explain several asp…

astro-ph.HE2024

The theory of resonant cosmic ray-driven instabilities -- Growth and saturation of single modes

Rouven Lemmerz, Mohamad Shalaby, Christoph Pfrommer +1

Cosmic ray (CR) feedback is critical for galaxy formation as CRs drive galactic winds, regularize star formation in galaxies, and escape from active galactic nuclei to heat the coo…