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

collaborators

18 papers

astro-ph.CO2009

Radiatively enhanced elasticity and turbulence in clumpy tori of Active Galactic Nuclei

Martin Krause, Marc Schartmann, Andreas Burkert +1

The paper assumes radiation forces proportional to distance between equal temperature clouds. However, we assume there are clouds in any direction. The forces then cancel almost en…

astro-ph2008★ 2 cited

Braneworlds with timelike extra-dimension

Marina Seikel, Max Camenzind

In this work, we consider a braneworld model with a timelike extra-dimension. There are strong constraints to the parameter values of such a model resulting from the claim that the…

astro-ph2008★ 212 cited

Three-dimensional radiative transfer models of clumpy tori in Seyfert galaxies

M. Schartmann, K. Meisenheimer, M. Camenzind +3

Tori of Active Galactic Nuclei are made up of a mixture of hot and cold gas, as well as dust. In order to protect the dust grains from destruction by the hot gas as well as by the…

astro-ph2008★ 6 cited

An implicit numerical algorithm for solving the general relativistic hydrodynamical equations around accreting compact objects

Ahmad Hujeirat, Max Camenzind, Bernhard W. Keil

An implicit algorithm for solving the equations of general relativistic hydrodynamics in conservative form in three-dimensional axi-symmetry is presented. This algorithm is a direc…

astro-ph2007

Large-scale Propagation of Very Light Jets in Galaxy Clusters

V. Gaibler, M. Camenzind, M. Krause

We performed MHD simulations of very light bipolar jets with density contrasts down to 10^-4 in axisymmetry, which were injected into a medium of constant density and evolved up to…

astro-ph2005★ 185 cited

Towards a physical model of dust tori in Active Galactic Nuclei - Radiative transfer calculations for a hydrostatic torus model

Marc Schartmann, Klaus Meisenheimer, Max Camenzind +2

We explore physically self-consistent models of dusty molecular tori in Active Galactic Nuclei (AGN) with the goal of interpreting VLTI observations and fitting high resolution mid…