Estudio infrarrojo de cúmulos inmersos en l = 345°

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dc.catalogadoryvc
dc.contributor.authorBaume, G.
dc.contributor.authorFeinstein, C.
dc.contributor.authorBorissova, J.
dc.contributor.authorKurtev, R.
dc.contributor.authorChené, A. -N.
dc.contributor.authorMoni Bidin, C.
dc.contributor.authorMauro, F.
dc.contributor.authorBonatto, C.
dc.contributor.authorBica, E.
dc.contributor.authorClarke, J. R. A.
dc.contributor.authorCatelan, Márcio
dc.contributor.authorGeisler, D.
dc.contributor.authorMinniti, D.
dc.contributor.authorLucas, P. W.
dc.date.accessioned2024-02-28T13:37:38Z
dc.date.available2024-02-28T13:37:38Z
dc.date.issued2011
dc.description.abstractWe have studied several embedded star clusters located in the fourth quad- rant of the Galactic plane (l 345 ; b +1.5 ). Data involves photometry and infrared spectroscopy (bands JHK and low dispersion respectively). This analysis has yielded a preliminary estimate of the fundamental param- eters of these objects and the behavior of the interstellar medium in this Galactic direction. FULL TEXT IN SPANISH...
dc.fuente.origenORCID
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81398
dc.information.autorucInstituto de Astrofísica ; Catelan, Márcio ; 0000-0001-6003-8877 ; 1001556
dc.language.isoen
dc.rightsacceso restringido
dc.titleEstudio infrarrojo de cúmulos inmersos en l = 345°
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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