Abundances of disk and bulge giants from high-resolution optical spectra II. O, Mg, Co, and Ti in the bulge sample

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dc.contributor.authorJönsson, H.
dc.contributor.authorRyde, N.
dc.contributor.authorSchultheis, M.
dc.contributor.authorZoccali, Manuela
dc.date.accessioned2020-07-23T15:51:21Z
dc.date.available2020-07-23T15:51:21Z
dc.date.issued2017
dc.fuente.origenConveris
dc.identifier.doi10.1051/0004-6361/201629129
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201629129
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/37002
dc.identifier.wosidWOS:000394465000100
dc.language.isoen
dc.nota.accesoContenido completo
dc.revistaAstronomy and Astrophysicses_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherFormación de Estrellases_ES
dc.subject.otherEstrellas - Evoluciónes_ES
dc.subject.otherGalaxiases_ES
dc.titleAbundances of disk and bulge giants from high-resolution optical spectra II. O, Mg, Co, and Ti in the bulge samplees_ES
dc.typeartículo
dc.volumenVol. 598
sipa.codpersvinculados1003159
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