Diffuse intracluster light at intermediate redshifts: intracluster light observations in an X-ray cluster at z= 0.29

dc.date.accessioned2020-03-11T20:36:48Z
dc.date.accessioned2022-10-18T23:04:33Z
dc.date.available2020-03-11T20:36:48Z
dc.date.available2022-10-18T23:04:33Z
dc.date.created2020-03-11T20:36:48Z
dc.date.issued2011
dc.identifierhttp://hdl.handle.net/10533/241102
dc.identifier15010003
dc.identifierWOS:000292141600066
dc.identifierno scielo
dc.identifiereid=2-s2.0-79957917274
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472441
dc.description.abstractThe diffuse intracluster light (ICL) contains a significant fraction of the total stellar mass in clusters of galaxies, and contributes in roughly equal proportion as the hot intra-cluster medium (ICM) to the total baryon content of clusters. Because of t
dc.languageeng
dc.relationhttps://doi.org/10.1111/j.1365-2966.2011.18423.x
dc.relation10.1111/j.1365-2966.2011.18423.x
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.titleDiffuse intracluster light at intermediate redshifts: intracluster light observations in an X-ray cluster at z= 0.29
dc.typeArticulo


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