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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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Bibliographische Detailangaben
Hauptverfasser: Pakmor, Rüdiger (VerfasserIn) , Guillet, Thomas (VerfasserIn) , Grand, Robert J. J. (VerfasserIn) , Springel, Volker (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2018 September 24
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 481, Heft: 4, Pages: 4410-4418
ISSN:1365-2966
DOI:10.1093/mnras/sty2601
Online-Zugang:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2601
Verlag, Volltext: https://academic.oup.com/mnras/article/481/4/4410/5106366
Volltext
Verfasserangaben:Rüdiger Pakmor, Thomas Guillet, Christoph Pfrommer, Facundo A. Gómez, Robert J.J. Grand, Federico Marinacci, Christine M. Simpson, and Volker Springel

MARC

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