METALS IN THE ICM: WITNESSES OF CLUSTER FORMATION AND EVOLUTION

The baryonic composition of galaxy clusters and groups is dominated by a hot, X-ray emitting Intra-Cluster Medium (ICM). The mean metallicity of the ICM has been found to be roughly 0.3 ÷ 0.5 times the solar value, therefore a large fraction of this gas cannot be of purely primordial origin. Indeed,...

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Main Authors: Lorenzo Lovisari, Tatiana F. Laganá, Katharina Borm, Gerrit Schellenberger, Thomas H. Reiprich
Format: Article
Language:English
Published: CTU Central Library 2013-12-01
Series:Acta Polytechnica
Online Access:https://ojs.cvut.cz/ojs/index.php/ap/article/view/1906
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spelling doaj-391173629c27437b9307a00dc3651faa2020-11-24T23:24:00ZengCTU Central LibraryActa Polytechnica1210-27091805-23632013-12-0153A10.14311/AP.2013.53.05791896METALS IN THE ICM: WITNESSES OF CLUSTER FORMATION AND EVOLUTIONLorenzo Lovisari0Tatiana F. Laganá1Katharina Borm2Gerrit Schellenberger3Thomas H. Reiprich4Argelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 BonnUniversidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Departamento de Astronomia, Cidade Universitária, CEP:05508-090, São PauloArgelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 BonnArgelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 BonnArgelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 BonnThe baryonic composition of galaxy clusters and groups is dominated by a hot, X-ray emitting Intra-Cluster Medium (ICM). The mean metallicity of the ICM has been found to be roughly 0.3 ÷ 0.5 times the solar value, therefore a large fraction of this gas cannot be of purely primordial origin. Indeed, the distribution and amount of metals in the ICM is a direct consequence of the past history of star formation in the cluster galaxies and of the processes responsible for the injection of enriched material into the ICM. We here shortly summarize the current views on the chemical enrichment, focusing on the observational evidence in terms of metallicity measurements in clusters, spatial metallicity distribution and evolution, and expectations from future missions.https://ojs.cvut.cz/ojs/index.php/ap/article/view/1906
collection DOAJ
language English
format Article
sources DOAJ
author Lorenzo Lovisari
Tatiana F. Laganá
Katharina Borm
Gerrit Schellenberger
Thomas H. Reiprich
spellingShingle Lorenzo Lovisari
Tatiana F. Laganá
Katharina Borm
Gerrit Schellenberger
Thomas H. Reiprich
METALS IN THE ICM: WITNESSES OF CLUSTER FORMATION AND EVOLUTION
Acta Polytechnica
author_facet Lorenzo Lovisari
Tatiana F. Laganá
Katharina Borm
Gerrit Schellenberger
Thomas H. Reiprich
author_sort Lorenzo Lovisari
title METALS IN THE ICM: WITNESSES OF CLUSTER FORMATION AND EVOLUTION
title_short METALS IN THE ICM: WITNESSES OF CLUSTER FORMATION AND EVOLUTION
title_full METALS IN THE ICM: WITNESSES OF CLUSTER FORMATION AND EVOLUTION
title_fullStr METALS IN THE ICM: WITNESSES OF CLUSTER FORMATION AND EVOLUTION
title_full_unstemmed METALS IN THE ICM: WITNESSES OF CLUSTER FORMATION AND EVOLUTION
title_sort metals in the icm: witnesses of cluster formation and evolution
publisher CTU Central Library
series Acta Polytechnica
issn 1210-2709
1805-2363
publishDate 2013-12-01
description The baryonic composition of galaxy clusters and groups is dominated by a hot, X-ray emitting Intra-Cluster Medium (ICM). The mean metallicity of the ICM has been found to be roughly 0.3 ÷ 0.5 times the solar value, therefore a large fraction of this gas cannot be of purely primordial origin. Indeed, the distribution and amount of metals in the ICM is a direct consequence of the past history of star formation in the cluster galaxies and of the processes responsible for the injection of enriched material into the ICM. We here shortly summarize the current views on the chemical enrichment, focusing on the observational evidence in terms of metallicity measurements in clusters, spatial metallicity distribution and evolution, and expectations from future missions.
url https://ojs.cvut.cz/ojs/index.php/ap/article/view/1906
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AT gerritschellenberger metalsintheicmwitnessesofclusterformationandevolution
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