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Remarks on Statistical Properties of the Turbulent Interstellar Medium
M. A. de Avillez, D. Breitschwerdt
The supernova-driven interstellar medium in star-forming galaxies has Reynolds numbers of the order of or even larger. We study, by means of adaptive mesh refinement hydro…
Ovi Column Density Distribution in the Local Bubble - Results from 3D Adaptive Mesh Refinement Simulations
Miguel A. de Avillez, Dieter Breitschwerdt
The Local Bubble (LB) is an X-ray emitting region extending 100 pc in radius in the Galactic plane and 300 pc perpendicular to it, and it is embedded in a somewhat larger H{\sc i}…
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…
Mixing of Primordial Elements in a Supernova-Driven ISM
Miguel A. de Avillez, Mordecai-Mark Mac Low
In order to understand the time scales for complete mixing in a supernova-driven ISM we used the model of Avillez (2000) to follow the mixing and dispersal of inhomogeneities with…
Three-Dimensional Evolution of the Galactic Fountain
Miguel A. de Avillez
Gas that escapes from the Galactic disk, rises into the halo, cools and falls back, constitutes a "Galactic Fountain". Three-Dimensional simulations show that such a fountain model…