X-ray and Radio Observations of the Radio Relic Galaxy Clusters 1RXS J0603.3+4214 and RXC J1053.7+5453

We study two galaxy clusters with radio relics, 1RXS J0603.3+4214 and RXC J1053.7+5453, through X-ray and radio observations. Radio relics are diffuse non-thermal radio sources found in outskirts of galaxy clusters. Because of their shape and location, they are thought to be related to cluster merge...

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Main Author: Motokazu Takizawa
Format: Article
Language:English
Published: MDPI AG 2018-12-01
Series:Galaxies
Subjects:
Online Access:http://www.mdpi.com/2075-4434/7/1/2
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author Motokazu Takizawa
author_facet Motokazu Takizawa
author_sort Motokazu Takizawa
collection DOAJ
description We study two galaxy clusters with radio relics, 1RXS J0603.3+4214 and RXC J1053.7+5453, through X-ray and radio observations. Radio relics are diffuse non-thermal radio sources found in outskirts of galaxy clusters. Because of their shape and location, they are thought to be related to cluster merger shocks. The galaxy cluster 1RXS J0603.3+4214 has a well-known linear-shape “toothbrush” radio relic. We investigate the temperature structure across the relic to constrain the Mach number of the associated shock. The results are compared with radio spectral results, which suggest that a simple diffusive shock acceleration model does not hold for this relic. The RXC J1053.7+5453 harbors a standard arc-like relic. We also get the Mach number from the temperature profile. In addition, we found an edge-like structure in the X-ray image between the X-ray peak and relic. We investigate the density and temperature profiles across the edge and found that the structure is likely relevant to not a shock but a contact discontinuity.
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spelling doaj.art-5d29b8e0aa184abba2334ca6b20683f12022-12-22T03:09:23ZengMDPI AGGalaxies2075-44342018-12-0171210.3390/galaxies7010002galaxies7010002X-ray and Radio Observations of the Radio Relic Galaxy Clusters 1RXS J0603.3+4214 and RXC J1053.7+5453Motokazu Takizawa0Department of Physics, Yamagata University, Kojirakawa-Machi 1-4-12, Yamagata, Yamagata 990-8560, JapanWe study two galaxy clusters with radio relics, 1RXS J0603.3+4214 and RXC J1053.7+5453, through X-ray and radio observations. Radio relics are diffuse non-thermal radio sources found in outskirts of galaxy clusters. Because of their shape and location, they are thought to be related to cluster merger shocks. The galaxy cluster 1RXS J0603.3+4214 has a well-known linear-shape “toothbrush” radio relic. We investigate the temperature structure across the relic to constrain the Mach number of the associated shock. The results are compared with radio spectral results, which suggest that a simple diffusive shock acceleration model does not hold for this relic. The RXC J1053.7+5453 harbors a standard arc-like relic. We also get the Mach number from the temperature profile. In addition, we found an edge-like structure in the X-ray image between the X-ray peak and relic. We investigate the density and temperature profiles across the edge and found that the structure is likely relevant to not a shock but a contact discontinuity.http://www.mdpi.com/2075-4434/7/1/2acceleration of particlesgalaxy clustersmagnetic fieldsshock waves
spellingShingle Motokazu Takizawa
X-ray and Radio Observations of the Radio Relic Galaxy Clusters 1RXS J0603.3+4214 and RXC J1053.7+5453
Galaxies
acceleration of particles
galaxy clusters
magnetic fields
shock waves
title X-ray and Radio Observations of the Radio Relic Galaxy Clusters 1RXS J0603.3+4214 and RXC J1053.7+5453
title_full X-ray and Radio Observations of the Radio Relic Galaxy Clusters 1RXS J0603.3+4214 and RXC J1053.7+5453
title_fullStr X-ray and Radio Observations of the Radio Relic Galaxy Clusters 1RXS J0603.3+4214 and RXC J1053.7+5453
title_full_unstemmed X-ray and Radio Observations of the Radio Relic Galaxy Clusters 1RXS J0603.3+4214 and RXC J1053.7+5453
title_short X-ray and Radio Observations of the Radio Relic Galaxy Clusters 1RXS J0603.3+4214 and RXC J1053.7+5453
title_sort x ray and radio observations of the radio relic galaxy clusters 1rxs j0603 3 4214 and rxc j1053 7 5453
topic acceleration of particles
galaxy clusters
magnetic fields
shock waves
url http://www.mdpi.com/2075-4434/7/1/2
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