activity
19962018
most citedCluster Magnetic Fields from Galactic Outflows

158 citations · 441 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2018★ 16 cited

Numerical Models for the Diffuse Ionized Gas in Galaxies. II. Three-dimensional radiative transfer in inhomogeneous interstellar structures as a tool for analyzing the diffuse ionized gas

J. A. Weber, A. W. A. Pauldrach, T. L. Hoffmann

Aims: We systematically explore a plausible subset of the parameter space involving effective temperatures and metallicities of the ionizing stellar sources, the effects of the har…

astro-ph.GA2013★ 129 cited

Cosmic rays can drive strong outflows from gas-rich high-redshift disk galaxies

Michal Hanasz, Harald Lesch, Thorsten Naab +3

We present simulations of the magnetized interstellar medium (ISM) in models of massive star forming (40 Msun / yr) disk galaxies with high gas surface densities (~100 Msun / pc^2)…

astro-ph.GA2012★ 14 cited

Numerical Models for the Diffuse Ionized Gas in Galaxies. I. Synthetic spectra of thermally excited gas with turbulent magnetic reconnection as energy source

T. L. Hoffmann, S. Lieb, A. W. A. Pauldrach +3

Aims: The aim of this work is to verify whether turbulent magnetic reconnection can provide the additional energy input required to explain the up to now only poorly understood ion…

astro-ph.CO2009★ 53 cited

Magnetic field structure due to the global velocity field in spiral galaxies

H. Kotarba, H. Lesch, K. Dolag +3

We present a set of global, self-consistent N-body/SPH simulations of the dynamic evolution of galactic discs with gas and including magnetic fields. We have implemented a descript…

astro-ph2008★ 158 cited

Cluster Magnetic Fields from Galactic Outflows

J. Donnert, K. Dolag, H. Lesch +1

We performed cosmological, magneto-hydrodynamical simulations to follow the evolution of magnetic fields in galaxy clusters, exploring the possibility that the origin of the magnet…

astro-ph2002★ 5 cited

Evolution and structure of magnetic fields in simulated galaxy clusters

Klaus Dolag, Matthias Bartelmann, Harald Lesch

We use cosmological magneto-hydrodynamic simulations to study the evolution of magnetic fields in galaxy clusters in two different cosmological models, a standard-CDM and a -CDM…