Modelling the supernova-driven ISM in different environments

We use hydrodynamical simulations in a (256 pc)3 periodic box to model the impact of supernova (SN) explosions on the multiphase interstellar medium (ISM) for initial densities n = 0.5-30 cm−3 and SN rates 1-720 Myr−1. We include radiative cooling, diffuse heating, and the formation of molecular gas...

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Bibliographic Details

Main Authors:	Gatto, Andrea (Author) , Glover, Simon (Author) , Klessen, Ralf S. (Author) , Clark, Paul C. (Author) , Baczynski, Christian (Author)
Format:	Article (Journal)
Language:	English
Published:	20 March 2015
In:	Monthly notices of the Royal Astronomical Society Year: 2015, Volume: 449, Issue: 1, Pages: 1057-1075
ISSN:	1365-2966
DOI:	10.1093/mnras/stv324
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stv324
Author Notes:	A. Gatto, S. Walch, M.-M. Mac Low, T. Naab, P. Girichidis, S.C.O. Glover, R. Wünsch, R.S. Klessen, P.C. Clark, C. Baczynski, T. Peters, J.P. Ostriker, J.C. Ibáñez-Mejía and S. Haid