Investigando cúmulos estelares masivos con el VVV

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dc.catalogadoryvc
dc.contributor.authorChené, A. -N.
dc.contributor.authorClarke, J. R. A.
dc.contributor.authorBorissova, J.
dc.contributor.authorMoni Bidin, C.
dc.contributor.authorMauro, F.
dc.contributor.authorBonatto, C.
dc.contributor.authorKurtev, R.
dc.contributor.authorBaume, G.
dc.contributor.authorFeinstein, C.
dc.contributor.authorMinniti, D.
dc.contributor.authorCatelan, Márcio
dc.contributor.authorLucas, P. W.
dc.contributor.authorGeisler, D.
dc.date.accessioned2024-02-28T13:37:38Z
dc.date.available2024-02-28T13:37:38Z
dc.date.issued2011
dc.description.abstractPreliminary results are presented for the study of infrared data of three mas- sive stellar clusters. Have been combined photometric observations (JHK; VVV project = Vista Variables in the Vía Láctea) and spectroscopic (follow- up) observations of the brightest stars in these clusters. In this way we have been able to refine the values of distance, reddening, age and masses of the involved objects. FULL TEXT IN SPANISH...
dc.fuente.origenORCID
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81399
dc.information.autorucInstituto de Astrofísica ; Catelan, Márcio ; 0000-0001-6003-8877 ; 1001556
dc.language.isoen
dc.rightsacceso restringido
dc.titleInvestigando cúmulos estelares masivos con el VVV
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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