{"title":"Infrared Observations of Galaxy Clusters","authors":"D. Elbaz","doi":"10.1017/S1539299600019754","DOIUrl":null,"url":null,"abstract":"The evolution of galaxy clusters from their formation due to the merging of sub structures, the bulk of star formation and subsequent chemical enrichment of the intra-cluster medium, is expected to be quite recent (z<1-2) in the hierarchical clustering scenario (White & Prenk 1991).","PeriodicalId":422890,"journal":{"name":"Highlights of Astronomy","volume":"2009 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1997-11-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Highlights of Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1017/S1539299600019754","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
The evolution of galaxy clusters from their formation due to the merging of sub structures, the bulk of star formation and subsequent chemical enrichment of the intra-cluster medium, is expected to be quite recent (z<1-2) in the hierarchical clustering scenario (White & Prenk 1991).