Properties of Polarized Synchrotron Emission from Fluctuation Dynamo Action—II. Effects of Turbulence Driving in the ICM and Beam Smoothing

Properties of Polarized Synchrotron Emission from Fluctuation Dynamo Action—II. Effects of Turbulence Driving in the ICM and Beam Smoothing

Polarized synchrotron emission from the radio halos of diffuse intracluster medium (ICM) in galaxy clusters are yet to be observed. To investigate the expected polarization in the ICM, we use high resolution (1 kpc) magnetohydrodynamic simulations of fluctuation dynamos, which produces intermittent...

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Bibliographic Details
Main Authors: Aritra Basu, Sharanya Sur
Format: Article
Language:English
Published: MDPI AG 2021-09-01
Series:Galaxies
Subjects:
intracluster magnetic fields
polarimetry
depolarization
magnetohydrodynamic simulations
Online Access:https://www.mdpi.com/2075-4434/9/3/62

Internet

https://www.mdpi.com/2075-4434/9/3/62

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