Characterizing the Uncertainty in Cluster Magnetic Fields Derived from Rotation Measures

Magnetic fields play vital roles in intracluster media (ICMs), but estimating their strengths and distributions from observations is a major challenge. Faraday rotation measures (RMs) are widely applied to this task, so it is critical to understand inherent uncertainties in RM analysis. In this pape...

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Vydané v:	The Astrophysical journal Ročník 888; číslo 2; s. 101 - 116
Hlavní autori:	Johnson, A. R., Rudnick, L., Jones, T. W., Mendygral, P. J., Dolag, K.
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Philadelphia The American Astronomical Society 10.01.2020 IOP Publishing
Predmet:	Astrophysics Computational fluid dynamics Computer simulation Electron density Extragalactic magnetic fields Faraday effect Field strength Fluid flow Galactic clusters Galaxies Galaxy clusters Intracluster medium Magnetic fields Magnetohydrodynamics Parameter uncertainty Physical properties Polarimetry Uncertainty analysis
ISSN:	0004-637X, 1538-4357
On-line prístup:	Získať plný text
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