New clues to the cause of extended main-sequence turnoffs in intermediate-age star clusters in the magellanic clouds

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dc.contributor.authorCorrenti, Matteo
dc.contributor.authorGoudfrooij, Paul
dc.contributor.authorKalirai, Jason S.
dc.contributor.authorGirardi, Leo
dc.contributor.authorPuzia, Thomas H.
dc.contributor.authorKerber, Leandro
dc.date.accessioned2021-06-04T14:25:37Z
dc.date.available2021-06-04T14:25:37Z
dc.date.issued2014
dc.format.extent9 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1088/0004-637X/793/2/121
dc.identifier.eissn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttps://doi.org/10.1088/0004-637X/793/2/121
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/60490
dc.issue.numeroNo. 2
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final9
dc.pagina.inicio1
dc.revistaAstrophysical Journales_ES
dc.rightsacceso abierto
dc.titleNew clues to the cause of extended main-sequence turnoffs in intermediate-age star clusters in the magellanic cloudses_ES
dc.typeartículo
dc.volumenVol. 793
sipa.codpersvinculados1008925
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