The Gaia -ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young-field stars

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dc.contributor.authorMagrini L.
dc.contributor.authorRandich S.
dc.contributor.authorKordopatis G.
dc.contributor.authorPrantzos N.
dc.contributor.authorRomano D.
dc.contributor.authorChieffi A.
dc.contributor.authorLimongi M.
dc.contributor.authorFrançois P.
dc.contributor.authorPancino E.
dc.contributor.authorFriel E.
dc.contributor.authorBragaglia A.
dc.contributor.authorTautvaišiene G.
dc.contributor.authorSpina L.
dc.contributor.authorOverbeek J.
dc.contributor.authorCantat-Gaudin T.
dc.contributor.authorDonati P.
dc.contributor.authorVallenari A.
dc.contributor.authorSordo R.
dc.contributor.authorJiménez-Esteban F.M.
dc.contributor.authorTang B.
dc.contributor.authorDrazdauskas A.
dc.contributor.authorSousa S.
dc.contributor.authorDuffau S.
dc.contributor.authorJofré P.
dc.contributor.authorGilmore G.
dc.contributor.authorFeltzing S.
dc.contributor.authorAlfaro E.
dc.contributor.authorBensby T.
dc.contributor.authorFlaccomio E.
dc.contributor.authorKoposov S.
dc.contributor.authorLanzafame A.
dc.contributor.authorSmiljanic R.
dc.contributor.authorBayo A.
dc.contributor.authorCarraro G.
dc.contributor.authorCasey A.R.
dc.contributor.authorCostado M.T.
dc.contributor.authorDamiani F.
dc.contributor.authorFranciosini E.
dc.contributor.authorHourihane A.
dc.contributor.authorLardo C.
dc.contributor.authorLewis J.
dc.contributor.authorMonaco L.
dc.contributor.authorMorbidelli L.
dc.contributor.authorSacco G.
dc.contributor.authorSbordone L.
dc.contributor.authorWorley C.C.
dc.contributor.authorZaggia S.
dc.date.accessioned2024-04-30T15:24:33Z
dc.date.available2024-04-30T15:24:33Z
dc.date.issued2017-07
dc.descriptionIndexación: Scopus
dc.description.abstractContext. The spatial distribution of elemental abundances in the disc of our Galaxy gives insights both on its assembly process and subsequent evolution, and on the stellar nucleogenesis of the different elements. Gradients can be traced using several types of objects as, for instance, (young and old) stars, open clusters, HII regions, planetary nebulae. Aims. We aim to trace the radial distributions of abundances of elements produced through different nucleosynthetic channels - the α-elements O, Mg, Si, Ca and Ti, and the iron-peak elements Fe, Cr, Ni and Sc - by use of the Gaia-ESO IDR4 results for open clusters and young-field stars. Methods. From the UVES spectra of member stars, we have determined the average composition of clusters with ages > 0.1 Gyr. We derived statistical ages and distances of field stars. We traced the abundance gradients using the cluster and field populations and compared them with a chemo-dynamical Galactic evolutionary model. Results. The adopted chemo-dynamical model, with the new generation of metallicity-dependent stellar yields for massive stars, is able to reproduce the observed spatial distributions of abundance ratios, in particular the abundance ratios of [O/Fe] and [Mg/Fe] in the inner disc (5 kpc <RGC< 7 kpc), with their differences, that were usually poorly explained by chemical evolution models. Conclusions. Oxygen and magnesium are often considered to be equivalent in tracing α-element abundances and in deducing, for example, the formation timescales of different Galactic stellar populations. In addition, often [α/Fe] is computed combining several α-elements. Our results indicate, as expected, a complex and diverse nucleosynthesis of the various α-elements, in particular in the high metallicity regimes, pointing towards a different origin of these elements and highlighting the risk of considering them as a single class with common features. © ESO, 2017.
dc.description.urihttps://www.aanda.org/articles/aa/full_html/2017/07/aa30294-16/aa30294-16.html
dc.identifier.citationAstronomy and Astrophysics Volume 6031 July 2017 Article number A2
dc.identifier.doi10.1051/0004-6361/201630294
dc.identifier.issn0004-6361
dc.identifier.urihttps://repositorio.unab.cl/handle/ria/56485
dc.language.isoen
dc.publisherEDP Sciences
dc.rights.licenseCC BY 4.0 DEED Atribución 4.0 Internacional
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/deed.es
dc.subjectGalaxy: abundances
dc.subjectOpen clusters and associations: general
dc.titleThe Gaia -ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young-field stars
dc.typeArtículo
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