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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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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1725562487338696704 |