activity
20002005
most citedRelativistic Outflows form Active Galactic Nuclei

2 citations · 4 across the 4 of their papers we have counts for

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6 papers · 1 filter

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-ph20051 cited

Evolution of the ISM and Galactic Activity

Volker Gaibler, Max Camenzind, Martin Krause

We study the effects of time-dependent mass injection and heating on the evolution of the interstellar medium (ISM) in elliptical galaxies. As the large and luminous ellipticals ha…

astro-ph20042 cited

Relativistic Outflows form Active Galactic Nuclei

Max Camenzind

The current popular model for launching, accelerating and collimating astrophysical jets is based on magnetohydrodynamics (MHD). AGN jets are most probably powered by energy extrac…

astro-ph20041 cited

Interaction of Jets with Galactic Winds

Martin Krause, Max Camenzind

We have used the vectorised and parallelised magnetohydrodynamics code NIRVANA on the NEC SX-5 and the new SX-6 installation in parallel mode to simulate the interaction of jets wi…

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-ph2000

Collimated outflows of rapidly rotating young stellar objects

E. Breitmoser, M. Camenzind

We present an analytical model for the magnetic flux surfaces for rapidly rotating magnetized young stellar objects which is based on ideal, stationary, axisymmetric magnetohydrody…