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dc.creatorPenaloza, F.
dc.creatorBorissova, J.
dc.creatorBonatto, C.
dc.creatorGeisler, D.
dc.creatorMinniti, D.
dc.date.accessioned2020-03-11T20:36:51Z
dc.date.available2020-03-11T20:36:51Z
dc.date.issued2012
dc.identifier.urihttp://hdl.handle.net/10533/241128
dc.description.abstractYoung massive clusters are usually deeply embedded in dust and gas. They represent excellent astrophysical laboratories for revealing the enigma of star formation processes and the early stages of stellar evolution. Wide-field infrared surveys are a moder
dc.language.isoeng
dc.relation.urihttps://doi.org/10.1007/978-3-642-22113-2_16
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleVVV Study of the Young Milky Way Star Clusters Mercer 35, 69 and 70
dc.typeArticulo
dc.identifier.folio15010003
dc.description.conicytprogramFONDAP
dc.rights.driverinfo:eu-repo/semantics/openAccess
dc.title.journalRevista Mexicana de Astronomía y Astrofísica
dc.type.driverinfo:eu-repo/semantics/article
dc.description.shortconicytprogramFONDAP
dc.type.openaireinfo:eu-repo/semantics/publishedVersion


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