New Metallicities of RR Lyrae Stars in ω Centauri: Evidence for a Non-He-enhanced Metal-intermediate Population

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dc.contributor.authorSollima, A.
dc.contributor.authorCatelan, Márcio
dc.contributor.authorMinniti, D.
dc.date.accessioned2017-04-25T19:28:29Z
dc.date.available2017-04-25T19:28:29Z
dc.date.issued2006
dc.fechaingreso.objetodigital2025-07-29
dc.identifier.doi10.1086/503099
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/20977
dc.identifier.urihttps://doi.org/10.1086/503099
dc.language.isoen
dc.nota.accesocontenido completo
dc.relation.isformatofAstrophysical Journal Vol. 640, no. 1 (2006), p. [L43]-L46
dc.revistaAstrophysical Journales_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas RR Lyraees_ES
dc.subject.otherEstrellas - Cúmulos globulareses_ES
dc.subject.otherAstronomía - Observacioneses_ES
dc.titleNew Metallicities of RR Lyrae Stars in ω Centauri: Evidence for a Non-He-enhanced Metal-intermediate Population
dc.typeartículo
dc.volumenVol. 640
sipa.codpersvinculados1001556
sipa.codpersvinculados100504
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