activity
20242026
collaborators

15 papers

astro-ph.GA2026

Simulating realistic radio morphologies of Fanaroff-Riley I jets in a self-regulating cool-core cluster

Léna Jlassi, Rainer Weinberger, Christoph Pfrommer +3

Active galactic nucleus (AGN) jets radiate radio synchrotron emission displaying a wide range of morphologies. At the same time, they provide heat to prevent cooling flows in cool-…

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.GA2026

Revisiting radio synchrotron diagnostics in star-forming galaxies

Maria Werhahn, Christoph Pfrommer, Philipp Girichidis +7

Radio continuum observations are widely used to study cosmic ray (CR) electron populations and transport processes in star-forming galaxies, but their interpretation relies on seve…

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

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.GA2026

Simulating cosmic ray electron spectra and radio emission from an AGN jet outburst in a cool-core cluster

Léna Jlassi, Rainer Weinberger, Christoph Pfrommer +3

Active galactic nucleus (AGN) powered jets can accelerate cosmic ray electrons, leading to the observed radio synchrotron emission. To simulate this emission, jet dynamics in galax…