Multiple populations in Galactic globular clusters from a Strömgren perspective

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dc.catalogadoryvc
dc.contributor.authorAlonso-García, J.
dc.contributor.authorCatelan, Márcio
dc.contributor.authorAmigo, P.
dc.contributor.authorCortés, C.
dc.contributor.authorKuehn, C. A.
dc.contributor.authorGrundahl, F.
dc.contributor.authorLópez, G.
dc.contributor.authorSalinas, R.
dc.contributor.authorSmith, H. A.
dc.contributor.authorStetson, P. B.
dc.contributor.authorSweigart, Allen V.
dc.contributor.authorValcarce, Aldo A. R.
dc.contributor.authorZoccali, M.
dc.date.accessioned2024-02-28T13:37:39Z
dc.date.available2024-02-28T13:37:39Z
dc.date.issued2014
dc.description.abstractOur view of the stellar populations in globular clusters has radically changed in the last years. Now we are coming to believe that all globular clusters host at least two distinct stellar populations. We present in this contribution preliminary results of a photometric survey we are currently conducting to disentangle photometrically the several populations in a significant number of Galactic globular clusters, using the Strömgren system, aiming to characterize their relative ratios and their radial distributions....
dc.fuente.origenORCID
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81401
dc.information.autorucInstituto de Astrofísica ; Catelan, Márcio ; 0000-0001-6003-8877 ; 1001556
dc.language.isoen
dc.nota.accesocontenido parcial
dc.rightsacceso restringido
dc.titleMultiple populations in Galactic globular clusters from a Strömgren perspective
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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