Interaction of Jets with Galactic Winds

  • Martin Krause
  • Max Camenzind
Conference paper


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 with a galactic wind that might be typical for the star-bursting radio-galaxies of the early universe.


Radio Galaxy Cool Flow Blue Wing Dense Shell Galactic Wind 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • Martin Krause
    • 1
  • Max Camenzind
    • 1
  1. 1.Landessternwarte KönigstuhlHeidelbergGermany

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