Near-IR period-luminosity relations for pulsating stars in ω Centauri (NGC 5139) (Corrigendum)

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dc.catalogadoryvc
dc.contributor.authorNavarrete, C.
dc.contributor.authorCatelan, Márcio
dc.contributor.authorContreras Ramos, Rodrigo
dc.contributor.authorAlonso-García, J.
dc.contributor.authorGran, F.
dc.contributor.authorDékány, I.
dc.contributor.authorMinniti, D.
dc.date.accessioned2024-02-28T13:37:34Z
dc.date.available2024-02-28T13:37:34Z
dc.date.issued2017
dc.description.abstractErratum for: "An incorrect zero point for the empirical period-luminosity-metallicity (PL-Z) relations for RR Lyrae (RRL) stars in ω Centauri (NGC 5139) was inadvertently reported in Table 2 and Eqs. (4) and (5) of our original paper. The corrected table and equations are given below. The actual analysis that is described in the paper was based on the correct zero points, and so all of the results reported in our original publication remain unchanged".
dc.fechaingreso.objetodigital2024-05-29
dc.fuente.origenORCID
dc.identifier.doi10.1051/0004-6361/201630102e
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201630102e
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81368
dc.identifier.wosidWOS:000413941300001
dc.information.autorucInstituto de Astrofísica ; Catelan, Márcio ; 0000-0001-6003-8877 ; 1001556
dc.language.isoen
dc.nota.accesoContenido completo
dc.rightsacceso abierto
dc.titleNear-IR period-luminosity relations for pulsating stars in ω Centauri (NGC 5139) (Corrigendum)
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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