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Non-ideal magnetohydrodynamics on a moving mesh

Abstract. In certain astrophysical systems, the commonly employed ideal magnetohydrodynamics (MHD) approximation breaks down. Here, we introduce novel explicit

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Bibliographic Details
Main Authors: Marinacci, Federico (Author) , Vogelsberger, Mark (Author) , Kannan, Rahul (Author) , Mocz, Philip (Author) , Pakmor, Rüdiger (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 2018 February 15
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 476, Issue: 2, Pages: 2476-2492
ISSN:1365-2966
DOI:10.1093/mnras/sty397
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty397
Verlag, Volltext: https://academic.oup.com/mnras/article/476/2/2476/4862483
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Author Notes:Federico Marinacci, Mark Vogelsberger, Rahul Kannan, Philip Mocz, Rüdiger Pakmor and Volker Springel
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Summary:Abstract. In certain astrophysical systems, the commonly employed ideal magnetohydrodynamics (MHD) approximation breaks down. Here, we introduce novel explicit
Item Description:Gesehen am 08.02.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty397

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