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Global MHD Modelling of the ISM - From large towards small scale turbulence
Miguel A. de Avillez, Dieter Breitschwerdt
Dealing numerically with the turbulent nature and non-linearity of the physical processes involved in the ISM requires the use of sophisticated numerical schemes coupled to HD and…
Overview of the ISM Phases: Evolution of Large and Small Scale Structures in 3D high resolution HD and MHD simulations
Dieter Breitschwerdt, Miguel A. de Avillez
We review recent 3D high resolution numerical HD and MHD studies of a multi-component and multi-phase ISM. The computational grid was chosen large enough in the disk to represent t…
Disk-Halo-Disk Circulation and the Evolution of the ISM - 3D HD and MHD Adaptive Mesh Refinement Simulations
M. A. de Avillez, Dieter Breitschwerdt
State of the art models of the ISM use adaptive mesh refinement to capture small scale structures, by refining on the fly those regions of the grid where density and pressure gradi…
Keynote Lecture: Galactic and Extragalactic Bubbles
D. Breitschwerdt, M. A. de Avillez, M. J. Freyberg
The observational and theoretical state of Galactic and extragalactic bubbles are reviewed. Observations of superbubbles are discussed, with some emphasis on nearby bubbles such as…