Stellar archaeology in the Milky Way Halo . Variable stars and stellar populations in the new Milky Way satellites discovered by the SDSS

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dc.catalogadormas
dc.contributor.authorMusella, I.
dc.contributor.authorClementini, G.
dc.contributor.authorRipepi, V.
dc.contributor.authorDall'Ora, M.
dc.contributor.authorMarconi, M.
dc.contributor.authorGreco, C.
dc.contributor.authorMoretti, M. I.
dc.contributor.authorKinemuchi, K.
dc.contributor.authorDi Fabrizio, L.
dc.contributor.authorSmith, H. A.
dc.contributor.authorKuehn, C.
dc.contributor.authorRodgers, C. T.
dc.contributor.authorBeers, T. C.
dc.contributor.authorCatelan, Marcio
dc.contributor.authorPritzl, B. J.
dc.date.accessioned2024-02-02T13:58:45Z
dc.date.available2024-02-02T13:58:45Z
dc.date.issued2010
dc.description.abstractWe summarize results from the photometric survey of the recently discovered faint Milky Way satellites: Bootes I, Coma, Ursa Major II, Canes Venatici I, Canes Venatici II and Leo IV. Our team is studying these systems to characterize their stellar populations and structural parameters, as well as their variable star content, with the aim of deriving hints on the formation process of the Galactic halo....
dc.fuente.origenORCID
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81275
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.nota.accesocontenido completo
dc.rightsacceso abierto
dc.titleStellar archaeology in the Milky Way Halo . Variable stars and stellar populations in the new Milky Way satellites discovered by the SDSS
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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