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• W3100613657 endingPage "A106" @default.
• W3100613657 startingPage "A106" @default.
• W3100613657 abstract "Context . Several works have found an increase of the abundances of the s -process neutron-capture elements in the youngest Galactic stellar populations. These trends provide important constraints on stellar and Galactic evolution and they need to be confirmed with large and statistically significant samples of stars spanning wide age and distance intervals. Aims . We aim to trace the abundance patterns and the time evolution of five s -process elements – two belonging to the first peak, Y and Zr, and three belonging to the second peak, Ba, La, and Ce – using the Gaia -ESO IDR 5 results for open clusters and disc stars. Methods . From the UVES spectra of cluster member stars, we determined the average composition of clusters with ages >0.1 Gyr. We derived statistical ages and distances of field stars, and we separated them into thin and thick disc populations. We studied the time-evolution and dependence on metallicity of abundance ratios using open clusters and field stars whose parameters and abundances were derived in a homogeneous way. Results . Using our large and homogeneous sample of open clusters, thin and thick disc stars, spanning an age range larger than 10 Gyr, we confirm an increase towards young ages of s -process abundances in the solar neighbourhood. These trends are well defined for open clusters and stars located nearby the solar position and they may be explained by a late enrichment due to significant contribution to the production of these elements from long-living low-mass stars. At the same time, we find a strong dependence of the s -process abundance ratios on the Galactocentric distance and on the metallicity of the clusters and field stars. Conclusions . Our results, derived from the largest and most homogeneous sample of s -process abundances in the literature, confirm the growth with decreasing stellar ages of the s -process abundances in both field and open cluster stars. At the same time, taking advantage of the abundances of open clusters located in a wide Galactocentric range, these results offer a new perspective on the dependence of the s -process evolution on the metallicity and star formation history, pointing to different behaviours at various Galactocentric distances." @default.
• W3100613657 created "2020-11-23" @default.
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• W3100613657 date "2018-09-01" @default.
• W3100613657 modified "2023-10-18" @default.
• W3100613657 title "The <i>Gaia</i>-ESO Survey: the origin and evolution of <i>s</i>-process elements" @default.
• W3100613657 cites W147232447 @default.
• W3100613657 cites W1533254904 @default.
• W3100613657 cites W1655407151 @default.
• W3100613657 cites W1805612153 @default.
• W3100613657 cites W1905650611 @default.
• W3100613657 cites W1924607551 @default.
• W3100613657 cites W1968807574 @default.
• W3100613657 cites W1968936583 @default.
• W3100613657 cites W1971108842 @default.
• W3100613657 cites W1973213041 @default.
• W3100613657 cites W1981675530 @default.
• W3100613657 cites W1996507000 @default.
• W3100613657 cites W2001646918 @default.
• W3100613657 cites W2002352647 @default.
• W3100613657 cites W2002388102 @default.
• W3100613657 cites W2006669101 @default.
• W3100613657 cites W2014019250 @default.
• W3100613657 cites W2026923307 @default.
• W3100613657 cites W2030212922 @default.
• W3100613657 cites W2032663410 @default.
• W3100613657 cites W2041434381 @default.
• W3100613657 cites W2044148938 @default.
• W3100613657 cites W2048905273 @default.
• W3100613657 cites W2053671107 @default.
• W3100613657 cites W2055427200 @default.
• W3100613657 cites W2058151487 @default.
• W3100613657 cites W2058562025 @default.
• W3100613657 cites W2064064721 @default.
• W3100613657 cites W2066453499 @default.
• W3100613657 cites W2072932889 @default.
• W3100613657 cites W2079825787 @default.
• W3100613657 cites W2085955275 @default.
• W3100613657 cites W2086074464 @default.
• W3100613657 cites W2088390163 @default.
• W3100613657 cites W2089630383 @default.
• W3100613657 cites W2091022272 @default.
• W3100613657 cites W2098592245 @default.
• W3100613657 cites W2099850984 @default.
• W3100613657 cites W2103165993 @default.
• W3100613657 cites W2103941552 @default.
• W3100613657 cites W2111817932 @default.
• W3100613657 cites W2119187754 @default.
• W3100613657 cites W2131999259 @default.
• W3100613657 cites W2136093157 @default.
• W3100613657 cites W2136742711 @default.

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