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

collaborators
Showing 2016 · astro-ph.GAShow all

8 papers · 2 filters

astro-ph.GA2016★ 50 cited

Increasing blackhole feedback induced quenching with anisotropic thermal conduction

Rahul Kannan, Mark Vogelsberger, Christoph Pfrommer +5

Feedback from central supermassive blackholes is often invoked to explain the low star formation rates in massive galaxies at the centers of galaxy clusters. However, the detailed…

astro-ph.GA2016★ 62 cited

Cosmic ray heating in cool core clusters - II. Self-regulation cycle and non-thermal emission

Svenja Jacob, Christoph Pfrommer

Self-regulated feedback by active galactic nuclei (AGNs) appears to be critical in balancing radiative cooling of the low-entropy gas at the centres of galaxy clusters and in regul…

astro-ph.GA2016★ 59 cited

Cosmic ray heating in cool core clusters - I. Diversity of steady state solutions

Svenja Jacob, Christoph Pfrommer

The absence of large cooling flows in cool core clusters appears to require self-regulated energy feedback by active galactic nuclei (AGNs) but the exact heating mechanism has not…

astro-ph.GA2016★ 112 cited

Cosmic ray-driven galactic winds: streaming or diffusion?

Joshua Wiener, Christoph Pfrommer, S. Peng Oh

Cosmic rays (CRs) have recently re-emerged as attractive candidates for mediating feedback in galaxies because of their long cooling timescales. They can have energy densities comp…

astro-ph.GA2016★ 141 cited

The role of cosmic ray pressure in accelerating galactic outflows

Christine M. Simpson, Ruediger Pakmor, Federico Marinacci +5

We study the formation of galactic outflows from supernova explosions (SNe) with the moving-mesh code AREPO in a stratified column of gas with a surface density similar to the Milk…

astro-ph.GA2016★ 2 cited

Galactic winds driven by isotropic and anisotropic cosmic ray diffusion in disk galaxies

Ruediger Pakmor, Christoph Pfrommer, Christine M. Simpson +1

The physics of cosmic rays (CR) is a promising candidate for explaining the driving of galactic winds and outflows. Recent galaxy formation simulations have demonstrated the need f…