Published in Space Science Reviews, 2012, Vol. 166, pp. 281-291.
astro-ph/1204.3648

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Abstract: We review progress in the development of physically realistic three dimensional simulated models of the galaxy. We consider the scales from star forming molecular clouds to the full spiral disc. Models are computed using hydrodynamic (HD) or magnetohydrodynamic (MHD) equations and may include cosmic ray or tracer particles. The range of dynamical scales between the full galaxy structure and the turbulent scales of supernova (SN) explosions and even cloud collapse to form stars, make it impossible with current computing tools and resources to resolve all of these in one model. We therefore consider a hierarchy of models and how they can be related to enhance our understanding of the complete galaxy.

Keywords: ISM - Simulations - Magnetohydrodynamic - MHD - Hydrodynamic - Supernova - Cosmic rays - Magnetic field - Galaxy

Table of Contents

• INTRODUCTION
• REVIEW OF GALAXY SIMULATIONS IN 3D
• Korpi
• de Avillez
• Balsara
• Hanasz
• Slyz
• Mac Low
• Piontek
• Joung
• Gressel
• SUMMARY
• REFERENCES