activity
20182026
most citedCosmic rays and non-thermal emission in simulated galaxies: III. probing cosmic ray calorimetry with radio spectra and the FIR-radio correlation

57 citations · 165 across the 16 of their papers we have counts for

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18 papers · 1 filter

astro-ph.GA2026

Same galaxy, different CGM: how the metal loading of galactic winds regulates the baryon cycle in Milky Way-mass galaxies

Prachi Khatri, Freeke van de Voort, Rebekka Bieri +5

The circumgalactic medium (CGM) is both the reservoir of gas that fuels star formation and galaxy growth, and the repository for the mass, energy, and metals expelled through stell…

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.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.GA20261 cited

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…

astro-ph.GA2025

Steady-State or Not? The Evolution of Cosmic Ray Electron Spectra in Galaxies

Maria Werhahn, Christoph Pfrommer, Joseph Whittingham +4

Cosmic ray (CR) electrons are key tracers of non-thermal processes in galaxies, yet their spectra are often modelled under the untested assumption of steady state between injection…

astro-ph.GA2025

Robust magnetic field estimates in star-forming galaxies with the equipartition formula in the absence of equipartition

H. -H. Sandy Chiu, Mateusz Ruszkowski, Maria Werhahn +2

The equipartition model is widely used to estimate magnetic field strength from synchrotron intensity in radio galaxies, yet the validity of its underlying assumptions remains unce…