Supernovae driven turbulence in the interstellar medium

@article{Gent2012SupernovaeDT,
  title={Supernovae driven turbulence in the interstellar medium},
  author={Frederick A. Gent},
  journal={arXiv: Astrophysics of Galaxies},
  year={2012}
}
  • F. Gent
  • Published 1 November 2012
  • Physics
  • arXiv: Astrophysics of Galaxies
I model the multi-phase interstellar medium (ISM) randomly heated and shocked by supernovae, with gravity, differential rotation and other parameters we understand to be typical of the solar neighbourhood. The simulations are 3D extending horizontally 1 x 1 kpc squared and vertically 2 kpc, symmetric about the galactic mid-plane. They routinely span gas number densities 1/10000 to 100 per cubic cm, temperatures 100 to 100 MK, speeds up to 10000 km/s and Mach number up to 25. Radiative cooling… 
Modelling supernova-driven turbulence
ABSTRACT High Mach number shocks are ubiquitous in interstellar turbulence. The Pencil Code is particularly well suited to the study of magnetohydrodynamics in weakly compressible turbulence and the
Scientific usage of the Pencil Code Search results using
  • Computer Science
  • 2020
TLDR
In the following the authors present the papers that are making use of the Pencil Code either for their own scientific work of those authors, or for code comparison purposes, although the topics are often overlapping.