Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment

Autores
Cora, Sofía Alejandra; Tornatore, Luca; Borgani, Stefano
Año de publicación
2005
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
The dependence of iron abundance on cluster temperature is subject to continuous debate. There are some evidences of decreasing abundances from ~0.7 to ~0.3 times the solar metallicity in the temperature range of ~3 — 10 keV, while a roughly constant value of ~0.3 times solar is claimed. Physical interpretation of these ambiguous observational results calls for robust theoretical models that can predict systematic trends for the enrichment of clusters of different masses.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Hybrid Model
Galaxy Cluster
Metal Enrichment
Cluster Temperature
Galaxy Formation
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/142767
Acceder
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network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical EnrichmentCora, Sofía AlejandraTornatore, LucaBorgani, StefanoCiencias AstronómicasHybrid ModelGalaxy ClusterMetal EnrichmentCluster TemperatureGalaxy FormationThe dependence of iron abundance on cluster temperature is subject to continuous debate. There are some evidences of decreasing abundances from ~0.7 to ~0.3 times the solar metallicity in the temperature range of ~3 — 10 keV, while a roughly constant value of ~0.3 times solar is claimed. Physical interpretation of these ambiguous observational results calls for robust theoretical models that can predict systematic trends for the enrichment of clusters of different masses.Facultad de Ciencias Astronómicas y Geofísicas2005-12info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf355-357http://sedici.unlp.edu.ar/handle/10915/142767enginfo:eu-repo/semantics/altIdentifier/isbn/978-3-540-71173-5info:eu-repo/semantics/altIdentifier/doi/10.1007/978-3-540-71173-5_59info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-11-12T10:56:51Zoai:sedici.unlp.edu.ar:10915/142767Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-11-12 10:56:52.238SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment
title Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment
spellingShingle Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment
Cora, Sofía Alejandra
Ciencias Astronómicas
Hybrid Model
Galaxy Cluster
Metal Enrichment
Cluster Temperature
Galaxy Formation
title_short Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment
title_full Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment
title_fullStr Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment
title_full_unstemmed Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment
title_sort Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment
dc.creator.none.fl_str_mv Cora, Sofía Alejandra
Tornatore, Luca
Borgani, Stefano
author Cora, Sofía Alejandra
author_facet Cora, Sofía Alejandra
Tornatore, Luca
Borgani, Stefano
author_role author
author2 Tornatore, Luca
Borgani, Stefano
author2_role author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Hybrid Model
Galaxy Cluster
Metal Enrichment
Cluster Temperature
Galaxy Formation
topic Ciencias Astronómicas
Hybrid Model
Galaxy Cluster
Metal Enrichment
Cluster Temperature
Galaxy Formation
dc.description.none.fl_txt_mv The dependence of iron abundance on cluster temperature is subject to continuous debate. There are some evidences of decreasing abundances from ~0.7 to ~0.3 times the solar metallicity in the temperature range of ~3 — 10 keV, while a roughly constant value of ~0.3 times solar is claimed. Physical interpretation of these ambiguous observational results calls for robust theoretical models that can predict systematic trends for the enrichment of clusters of different masses.
Facultad de Ciencias Astronómicas y Geofísicas
description The dependence of iron abundance on cluster temperature is subject to continuous debate. There are some evidences of decreasing abundances from ~0.7 to ~0.3 times the solar metallicity in the temperature range of ~3 — 10 keV, while a roughly constant value of ~0.3 times solar is claimed. Physical interpretation of these ambiguous observational results calls for robust theoretical models that can predict systematic trends for the enrichment of clusters of different masses.
publishDate 2005
dc.date.none.fl_str_mv 2005-12
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
Objeto de conferencia
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/142767
url http://sedici.unlp.edu.ar/handle/10915/142767
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/isbn/978-3-540-71173-5
info:eu-repo/semantics/altIdentifier/doi/10.1007/978-3-540-71173-5_59
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
355-357
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.24909

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