Formation of multiple populations in globular clusters: another possible scenario

dc.date.accessioned2020-03-11T20:36:26Z
dc.date.accessioned2022-10-18T23:03:33Z
dc.date.available2020-03-11T20:36:26Z
dc.date.available2022-10-18T23:03:33Z
dc.date.created2020-03-11T20:36:26Z
dc.date.issued2011
dc.identifierhttp://hdl.handle.net/10533/240970
dc.identifier15010003
dc.identifierWOS:000295168100120
dc.identifierno scielo
dc.identifiereid=2-s2.0-84983643611
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472309
dc.description.abstractAims. While spreads in chemical composition are now believed to be a universal characteristic of globular clusters (GCs), not all of them display evidence of multiple populations in their color-magnitude diagrams (CMDs). Here we present a new scenario for
dc.languageeng
dc.relationhttps://doi.org/10.1051/0004-6361/201116955
dc.relation10.1051/0004-6361/201116955
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.titleFormation of multiple populations in globular clusters: another possible scenario
dc.typeArticulo


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