Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics

Autores
Stasyszyn, Federico Andres; de Los Rios, Martín Emilio
Año de publicación
2019
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We study the magnetic fields in galaxy clusters through Faraday rotation measurements crossing systems in different dynamical states. We confirm that magnetic fields are present in those systems and analyse the difference between relaxed and unrelaxed samples with respect to the dispersion between their inherent Faraday rotation measurements (RM). We found an increase of this RM dispersion and a higher RM overlapping frequency for unrelaxed clusters. This fact suggests that a large-scale physical process is involved in the nature of unrelaxed systems and possible depolarization effects are present in the relaxed ones. We show that dynamically unrelaxed systems can enhance magnetic fields to large coherence lengths. In contrast, the results for relaxed systems suggests that a small-scale dynamo can be a dominant mechanism for sustaining magnetic fields, leading to intrinsic depolarization.
Fil: Stasyszyn, Federico Andres. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: de Los Rios, Martín Emilio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Materia
GALAXIES: CLUSTERS: INTRACLUSTER MEDIUM
HYDRODYNAMICS
MAGNETIC FIELDS
METHODS: STATISTICAL
TURBULENCE
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/123815
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Faraday Rotation Measure Dependence on Galaxy Clusters DynamicsStasyszyn, Federico Andresde Los Rios, Martín EmilioGALAXIES: CLUSTERS: INTRACLUSTER MEDIUMHYDRODYNAMICSMAGNETIC FIELDSMETHODS: STATISTICALTURBULENCEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study the magnetic fields in galaxy clusters through Faraday rotation measurements crossing systems in different dynamical states. We confirm that magnetic fields are present in those systems and analyse the difference between relaxed and unrelaxed samples with respect to the dispersion between their inherent Faraday rotation measurements (RM). We found an increase of this RM dispersion and a higher RM overlapping frequency for unrelaxed clusters. This fact suggests that a large-scale physical process is involved in the nature of unrelaxed systems and possible depolarization effects are present in the relaxed ones. We show that dynamically unrelaxed systems can enhance magnetic fields to large coherence lengths. In contrast, the results for relaxed systems suggests that a small-scale dynamo can be a dominant mechanism for sustaining magnetic fields, leading to intrinsic depolarization.Fil: Stasyszyn, Federico Andres. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: de Los Rios, Martín Emilio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaWiley Blackwell Publishing, Inc2019-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/123815Stasyszyn, Federico Andres; de Los Rios, Martín Emilio; Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 487; 4; 8-2019; 4768-47740035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/487/4/4768/5525024info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stz1450info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1905.10303info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:47:05Zoai:ri.conicet.gov.ar:11336/123815instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:47:05.806CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
title Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
spellingShingle Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
Stasyszyn, Federico Andres
GALAXIES: CLUSTERS: INTRACLUSTER MEDIUM
HYDRODYNAMICS
MAGNETIC FIELDS
METHODS: STATISTICAL
TURBULENCE
title_short Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
title_full Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
title_fullStr Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
title_full_unstemmed Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
title_sort Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
dc.creator.none.fl_str_mv Stasyszyn, Federico Andres
de Los Rios, Martín Emilio
author Stasyszyn, Federico Andres
author_facet Stasyszyn, Federico Andres
de Los Rios, Martín Emilio
author_role author
author2 de Los Rios, Martín Emilio
author2_role author
dc.subject.none.fl_str_mv GALAXIES: CLUSTERS: INTRACLUSTER MEDIUM
HYDRODYNAMICS
MAGNETIC FIELDS
METHODS: STATISTICAL
TURBULENCE
topic GALAXIES: CLUSTERS: INTRACLUSTER MEDIUM
HYDRODYNAMICS
MAGNETIC FIELDS
METHODS: STATISTICAL
TURBULENCE
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We study the magnetic fields in galaxy clusters through Faraday rotation measurements crossing systems in different dynamical states. We confirm that magnetic fields are present in those systems and analyse the difference between relaxed and unrelaxed samples with respect to the dispersion between their inherent Faraday rotation measurements (RM). We found an increase of this RM dispersion and a higher RM overlapping frequency for unrelaxed clusters. This fact suggests that a large-scale physical process is involved in the nature of unrelaxed systems and possible depolarization effects are present in the relaxed ones. We show that dynamically unrelaxed systems can enhance magnetic fields to large coherence lengths. In contrast, the results for relaxed systems suggests that a small-scale dynamo can be a dominant mechanism for sustaining magnetic fields, leading to intrinsic depolarization.
Fil: Stasyszyn, Federico Andres. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: de Los Rios, Martín Emilio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
description We study the magnetic fields in galaxy clusters through Faraday rotation measurements crossing systems in different dynamical states. We confirm that magnetic fields are present in those systems and analyse the difference between relaxed and unrelaxed samples with respect to the dispersion between their inherent Faraday rotation measurements (RM). We found an increase of this RM dispersion and a higher RM overlapping frequency for unrelaxed clusters. This fact suggests that a large-scale physical process is involved in the nature of unrelaxed systems and possible depolarization effects are present in the relaxed ones. We show that dynamically unrelaxed systems can enhance magnetic fields to large coherence lengths. In contrast, the results for relaxed systems suggests that a small-scale dynamo can be a dominant mechanism for sustaining magnetic fields, leading to intrinsic depolarization.
publishDate 2019
dc.date.none.fl_str_mv 2019-08
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/123815
Stasyszyn, Federico Andres; de Los Rios, Martín Emilio; Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 487; 4; 8-2019; 4768-4774
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/123815
identifier_str_mv Stasyszyn, Federico Andres; de Los Rios, Martín Emilio; Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 487; 4; 8-2019; 4768-4774
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/487/4/4768/5525024
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stz1450
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1905.10303
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 12.982451

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