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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…
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…
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…
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…
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…
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…