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Faraday rotation maps of disc galaxies

ABSTRACT. Faraday rotation is one of the most widely used observables to infer the strength and configuration of the magnetic field in the ionized gas of the M

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Bibliographic Details
Main Authors: Pakmor, Rüdiger (Author) , Guillet, Thomas (Author) , Grand, Robert J. J. (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 2018 September 24
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 481, Issue: 4, Pages: 4410-4418
ISSN:1365-2966
DOI:10.1093/mnras/sty2601
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2601
Verlag, Volltext: https://academic.oup.com/mnras/article/481/4/4410/5106366
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Author Notes:Rüdiger Pakmor, Thomas Guillet, Christoph Pfrommer, Facundo A. Gómez, Robert J.J. Grand, Federico Marinacci, Christine M. Simpson, and Volker Springel
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Summary:ABSTRACT. Faraday rotation is one of the most widely used observables to infer the strength and configuration of the magnetic field in the ionized gas of the M
Item Description:Gesehen am 23.01.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty2601

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