On the interpretation of sub-giant branch morphologies of intermediate-age star clusters with extended main sequence turnoffs

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dc.contributor.authorGoudfrooij, P.
dc.contributor.authorGirardi, L.
dc.contributor.authorRosenfield, P.
dc.contributor.authorBressan, A.
dc.contributor.authorMarigo, P.
dc.contributor.authorCorrenti, M.
dc.contributor.authorPuzia, Thomas H.
dc.date.accessioned2021-01-26T18:30:14Z
dc.date.available2021-01-26T18:30:14Z
dc.date.issued2015
dc.format.extent12 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1093/mnras/stv700
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1093/mnras/stv700
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/52427
dc.issue.numeroNo. 2
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final1704
dc.pagina.inicio1693
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso abierto
dc.titleOn the interpretation of sub-giant branch morphologies of intermediate-age star clusters with extended main sequence turnoffses_ES
dc.typeartículo
dc.volumenVol. 450
sipa.codpersvinculados1008925
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