The HST/ACS Coma Cluster Survey. IV. Intergalactic Globular Clusters and the Massive Globular Cluster System at the Core of the Coma Galaxy Cluster

dc.date.accessioned2020-03-11T20:36:20Z
dc.date.accessioned2022-10-18T23:03:23Z
dc.date.available2020-03-11T20:36:20Z
dc.date.available2022-10-18T23:03:23Z
dc.date.created2020-03-11T20:36:20Z
dc.date.issued2011
dc.identifierhttp://hdl.handle.net/10533/240949
dc.identifier15010003
dc.identifierWOS:000288453600023
dc.identifierno scielo
dc.identifiereid=2-s2.0-79953725755
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472288
dc.description.abstractIntracluster stellar populations are a natural result of tidal interactions in galaxy clusters. Measuring these populations is difficult, but important for understanding the assembly of the most massive galaxies. The Coma cluster is one of the nearest tru
dc.languageeng
dc.relationhttps://doi.org/10.1088/0004-637X/730/1/23
dc.relation10.1088/0004-637X/730/1/23
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleThe HST/ACS Coma Cluster Survey. IV. Intergalactic Globular Clusters and the Massive Globular Cluster System at the Core of the Coma Galaxy Cluster
dc.typeArticulo


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