On a new Near-Infrared Method to Estimate the Absolute Ages of Star Clusters: NGC3201 as a First Test Case

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dc.contributor.authorBono, G.
dc.contributor.authorZoccali, Manuela
dc.date.accessioned2016-05-10T18:16:57Z
dc.date.available2016-05-10T18:16:57Z
dc.date.issued2010
dc.identifier.doi10.1088/2041-8205/708/2/L74
dc.identifier.issn2041-8205
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/14323
dc.identifier.wosidWOS:000273308000002
dc.language.isoen
dc.nota.accesoContenido completo
dc.relation.isformatofThe Astrophysical Journal Letters Vol. 708, No. 2, p. L74-L79.
dc.revistaThe Astrophysical Journal Letterses_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas - Cúmulos globulareses_ES
dc.subject.otherEstrellas - Evoluciónes_ES
dc.subject.otherAstrofísicaes_ES
dc.titleOn a new Near-Infrared Method to Estimate the Absolute Ages of Star Clusters: NGC3201 as a First Test Casees_ES
dc.typeartículo
dc.volumenVol. 708
sipa.codpersvinculados1003159
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