Population Parameters of Intermediate-age Star Clusters in the Large Magellanic Cloud. III. Dynamical Evidence for a Range of Ages Being Responsible for Extended Main-sequence Turnoffs

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dc.contributor.authorGoudfrooij, P.
dc.contributor.authorPuzia, Thomas H.
dc.date.accessioned2016-05-10T18:02:17Z
dc.date.available2016-05-10T18:02:17Z
dc.date.issued2011
dc.identifier.doi10.1088/0004-637X/737/1/4
dc.identifier.issn0004-637X
dc.identifier.urihttps://doi.org/10.1088/0004-637X/737/1/4
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/12185
dc.identifier.wosidWOS:000293332200004
dc.language.isoen
dc.nota.accesocontenido completo
dc.relation.isformatofAstrophysical Journal Vol. 737, No. 1, p. 1-10.
dc.revistaAstrophysical Journales_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas - Cúmulos Estrellas - Masases_ES
dc.subject.otherNubes magallánicases_ES
dc.subject.otherAstronomía - Observacioneses_ES
dc.titlePopulation Parameters of Intermediate-age Star Clusters in the Large Magellanic Cloud. III. Dynamical Evidence for a Range of Ages Being Responsible for Extended Main-sequence Turnoffses_ES
dc.typeartículo
dc.volumenVol. 737
sipa.codpersvinculados1008925
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