Launching cosmic-ray-driven outflows from the magnetized interstellar medium

We present a hydrodynamical simulation of the turbulent, magnetized, supernova (SN)-driven interstellar medium (ISM) in a stratified box that dynamically couples the injection and evolution of cosmic rays (CRs) and a self-consistent evolution of the chemical composition. CRs are treated as a relativ...

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Bibliographic Details

Main Authors:	Girichidis, Philipp (Author) , Naab, Thorsten (Author) , Walch, Stefanie (Author) , Hanasz, Michal (Author) , Mac Low, Mordecai-Mark (Author) , Ostriker, Jeremiah P. (Author) , Gatto, Andrea (Author) , Peters, Thomas (Author) , Wünsch, Richard (Author) , Glover, Simon (Author) , Klessen, Ralf S. (Author) , Clark, Paul C. (Author) , Baczynski, Christian (Author)
Format:	Article (Journal)
Language:	English
Published:	6 Jan 2016
In:	The astrophysical journal. Part 2, Letters Year: 2016, Volume: 816, Issue: 2, Pages: L19
ISSN:	2041-8213
DOI:	10.3847/2041-8205/816/2/L19
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.3847/2041-8205/816/2/L19 Verlag, lizenzpflichtig, Volltext: http://arxiv.org/abs/1509.07247
Author Notes:	Philipp Girichidis, Thorsten Naab, Stefanie Walch, Michal Hanasz, Mordecai-Mark Mac Low, Jeremiah P. Ostriker, Andrea Gatto, Thomas Peters, Richard Wünsch, Simon C. O. Glover, Ralf S. Klessen, Paul C. Clark, Christian Baczynski