Chemical abundances of 11 bulge stars from high-resolution, near-IR spectra

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dc.contributor.authorRyde, N.
dc.contributor.authorMinniti, D.
dc.contributor.authorZoccali, Manuela
dc.date.accessioned2016-05-10T18:02:09Z
dc.date.available2016-05-10T18:02:09Z
dc.date.issued2010
dc.identifier.doi10.1051/0004-6361/200912687
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361/200912687
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/12117
dc.language.isoen
dc.relation.isformatofAstronomy & Astrophysics No. 1 (509), p. 20.
dc.revistaAstronomy and Astrophysicses_ES
dc.rightsacceso restringido
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherVía Lácteaes_ES
dc.subject.otherFormación de Estrellases_ES
dc.subject.otherEstrellas - Cúmuloses_ES
dc.subject.otherAstronomía - Observacioneses_ES
dc.titleChemical abundances of 11 bulge stars from high-resolution, near-IR spectraes_ES
dc.typeartículo
sipa.codpersvinculados100504
sipa.codpersvinculados1003159
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