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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/123815
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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 Técnicas2025-09-29T10:16:55Zoai: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:34982025-09-29 10:16:56.114CONICET 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 |
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CONICET Digital (CONICET) |
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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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13.070432 |