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The impact of magnetic fields on the chemical evolution of the supernova-driven ISM

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Abstract: We present three-dimensional magneto-hydrodynamical simulations of the self-gravitating interstellar medium (ISM) in a periodic (256 pc)3 box with a mean number density of 0.5 cm−3. At a fixed supernova rate we investigate the multi-phase ISM structure, H2 molecule formation and density-ma...

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Main Authors: Pardi, Anabele-Linda (Author) , Glover, Simon (Author) , Klessen, Ralf S. (Author)
Format: Article (Journal)
Language:English
Published: 2017
In: Monthly notices of the Royal Astronomical Society
Year: 2016, Volume: 465, Issue: 4, Pages: 4611-4633
ISSN:1365-2966
DOI:10.1093/mnras/stw3071
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw3071
Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/465/4/4611/2608772
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Author Notes:A. Pardi, P. Girichidis, T. Naab, S. Walch, T. Peters, F. Heitsch, S.C.O. Glover, R S. Klessen, R. Wünsch and A. Gatto
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The impact of magnetic fields on the chemical evolution of the supernova-driven ISM by Pardi, Anabele-Linda (Author) , Glover, Simon (Author) , Klessen, Ralf S. (Author) ,


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