Abundance ratios of red giants in low-mass ultra-faint dwarf spheroidal galaxies

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dc.contributor.authorFrancois, P.
dc.contributor.authorMonaco, L.
dc.contributor.authorBonifacio, P.
dc.contributor.authorMoni Bidin, C.
dc.contributor.authorGeisler, D.
dc.contributor.authorSbordone, L.
dc.date.accessioned2025-01-23T21:31:41Z
dc.date.available2025-01-23T21:31:41Z
dc.date.issued2016
dc.description.abstractContext. Low-mass dwarf spheroidal galaxies are key objects for our understanding of the chemical evolution of the pristine Universe and the Local Group of galaxies. Abundance ratios in stars of these objects can be used to better understand their star formation and chemical evolution.
dc.description.abstractAims. We report on the analysis of a sample of 11 stars belonging to five different ultra-faint dwarf spheroidal galaxies (UfDSph) that is based on X-Shooter spectra obtained at the VLT.
dc.description.abstractMethods. Medium-resolution spectra have been used to determine the detailed chemical composition of their atmosphere. We performed a standard 1D LTE analysis to compute the abundances.
dc.description.abstractResults. Considering all the stars as representative of the same population of low-mass galaxies, we found that the [alpha/Fe] ratios vs.s [Fe/H] decreases as the metallicity of the star increases in a way similar to that which is found for the population of stars that belong to dwarf spheroidal galaxies. The main difference is that the solar [alpha/Fe] is reached at a much lower metallicity for the UfDSph than for the dwarf spheroidal galaxies. We report for the first time the abundance of strontium in CVn II. The star we analyzed in this galaxy has a very high [Sr/Fe] and a very low upper limit of barium which makes it a star with an exceptionally high [Sr/Ba] ratio.
dc.fuente.origenWOS
dc.identifier.doi10.1051/0004-6361/201527181
dc.identifier.eissn1432-0746
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201527181
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/101474
dc.identifier.wosidWOS:000373207800019
dc.language.isoen
dc.revistaAstronomy & astrophysics
dc.rightsacceso restringido
dc.subjectgalaxies: abundances
dc.subjectstars: abundances
dc.subjectLocal Group
dc.titleAbundance ratios of red giants in low-mass ultra-faint dwarf spheroidal galaxies
dc.typeartículo
dc.volumen588
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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