Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid

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dc.contributor.authorRazera, R.
dc.contributor.authorBarbuy, B.
dc.contributor.authorMoura, T. C.
dc.contributor.authorErnandes, H.
dc.contributor.authorPerez-Villegas, A.
dc.contributor.authorSouza, S. O.
dc.contributor.authorChiappini, C.
dc.contributor.authorQueiroz, A. B. A.
dc.contributor.authorAnders, F.
dc.contributor.authorFernandez-Trincado, J. G.
dc.contributor.authorFriaca, A. C. S.
dc.contributor.authorCunha, K.
dc.contributor.authorSmith, V. V.
dc.contributor.authorSantiago, B. X.
dc.contributor.authorSchiavon, R. P.
dc.contributor.authorValentini, M.
dc.contributor.authorMinniti, D.
dc.contributor.authorSchultheis, M.
dc.contributor.authorGeisler, D.
dc.contributor.authorSobeck, J.
dc.contributor.authorPlacco, V. M.
dc.contributor.authorZoccali, M.
dc.date.accessioned2025-01-20T21:01:35Z
dc.date.available2025-01-20T21:01:35Z
dc.date.issued2022
dc.description.abstractThe central part of the Galaxy hosts a multitude of stellar populations, including the spheroidal bulge stars, stars moved to the bulge through secular evolution of the bar, inner halo, inner thick disc, inner thin disc, as well as debris from past accretion events. We identified a sample of 58 candidate stars belonging to the stellar population of the spheroidal bulge, and analyse their abundances. The present calculations of Mg, Ca, and Si lines are in agreement with the ASPCAP abundances, whereas abundances of C, N, O, and Ce are re-examined. We find normal alpha-element enhancements in oxygen, similar to magnesium, Si, and Ca abundances, which are typical of other bulge stars surveyed in the optical in Baade's Window. The enhancement of [O/Fe] in these stars suggests that they do not belong to accreted debris. No spread in N abundances is found, and none of the sample stars is N-rich, indicating that these stars are not second generation stars originated in globular clusters. Ce instead is enhanced in the sample stars, which points to an s-process origin such as due to enrichment from early generations of massive fast rotating stars, the so-called spinstars.
dc.fuente.origenWOS
dc.identifier.doi10.1093/mnras/stac2136
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stac2136
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/92917
dc.identifier.wosidWOS:000878766100002
dc.issue.numero3
dc.language.isoen
dc.pagina.final4606
dc.pagina.inicio4590
dc.revistaMonthly notices of the royal astronomical society
dc.rightsacceso restringido
dc.subjectstars: abundances
dc.subjectstars: atmospheres
dc.subjectGalaxy: bulge
dc.titleAbundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid
dc.typeartículo
dc.volumen517
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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