ON THE AGES OF THE GALACTIC CLUSTERS NGC 188 M67 AND NGC 6791

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dc.contributor.authorTORRES PEIMBERT, S
dc.date.accessioned2026-05-28T15:48:14Z
dc.date.issued1953
dc.description.abstractTheoretical isochrones for three chemical compositions are presented and compared to the color-magnitude diagrams of NGC 188, M67 and NGC 6791. The metal abundances that provide the best agreement between theory and observations for NGC 188 are in the ran
dc.description.paginacion3 - 14
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent12
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/18760
dc.language.isoEspañol
dc.numero.secuencia18757
dc.publisherUNAM, Boletín de Observatorios Tonatzintla y Tacubaya, México.
dc.publisherDF
dc.relation.ispartofseriesVol. 6 No. 36
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectAGES, GALACTIC, CLUSTERS, NGC 188, M67, NGC 6791
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaGALAXIAS
dc.titleON THE AGES OF THE GALACTIC CLUSTERS NGC 188 M67 AND NGC 6791
dc.title.alternativeBOL OBS TONAN TACUB

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