Stellar populations of the newly discovered satellites of the Milky Way .

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dc.catalogadormas
dc.contributor.authorDall'Ora, M.
dc.contributor.authorClementini, G.
dc.contributor.authorRipepi, V.
dc.contributor.authorKinemuchi, K.
dc.contributor.authorGreco, C.
dc.contributor.authorKuehn, C.
dc.contributor.authorMusella, I.
dc.contributor.authorRodgers, C. T.
dc.contributor.authorDi Fabrizio, L.
dc.contributor.authorBeers, T. C.
dc.contributor.authorCatelan, Marcio
dc.contributor.authorMarconi, M.
dc.contributor.authorPritzl, B. J.
dc.contributor.authorSmith., H. A.
dc.date.accessioned2024-02-02T13:58:45Z
dc.date.available2024-02-02T13:58:45Z
dc.date.issued2008
dc.description.abstractWe have carried out an extensive observing campaign on the new dwarf spheroidal galaxies (dSphs) recently discovered by the SDSS, with the aim of characterizing their stellar populations and structural properties, as well as their variable star content. First preliminary results are presented for the Canes Venatici II, the Coma and the Ursa Major II dSphs, based on data collected at a variety of telescopes, and reaching each galaxy's Main Sequence Turn-Off (MSTO)....
dc.fuente.origenORCID
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81276
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.nota.accesocontenido completo
dc.rightsacceso abierto
dc.titleStellar populations of the newly discovered satellites of the Milky Way .
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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