activity
20002009
most citedThree-dimensional radiative transfer models of clumpy tori in Seyfert galaxies

212 citations · 569 across the 18 of their papers we have counts for

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Showing 2003Show all

5 papers · 1 filter

astro-ph2003★ 38 cited

Relativistic emission lines from accreting black holes - The effect of disk truncation on line profiles

Andreas Mueller, Max Camenzind

Relativistic emission lines generated by thin accretion disks around rotating black holes are an important diagnostic tool for testing gravity near the horizon. The iron K-line is…

astro-ph2003

Large Scale Simulations of Jets in Dense and Magnetised Environments

Martin G. H. Krause, Max Camenzind

We report two simulations that have been carried out at the SX-5 at HLRS (Stuttgart). One simulation is axisymmetric and purely hydrodynamic, but with a resolution of 20 points per…

astro-ph2003★ 33 cited

Towards a self-consistent relativistic model of the exterior gravitational field of rapidly rotating neutron stars

Matthias Stute, Max Camenzind

We present a self-consistent, relativistic model of rapidly rotating neutron stars describing their exterior gravitational field. This is achieved by matching the new solution of E…

astro-ph2003★ 22 cited

Parameters for Very Light Jets of cD Galaxies

Martin Krause, Max Camenzind

Recent Chandra X-ray observations of jets in central cluster galaxies show interesting features around the symmetry plane. We have carried out simulations involving bipolar jets, r…

astro-ph2003★ 37 cited

Evolution of bimodal accretion flows

J. Gracia, J. Peitz, Ch. Keller +1

We consider time-dependent models for rotating accretion flows onto black holes, where a transition takes place from an outer cooling-dominated disc to a radiatively inefficient fl…