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20052026
most citedThe Gaia-ESO Survey: the Galactic Thick to Thin Disc transition

241 citations · 5.5k across the 134 of their papers we have counts for

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Showing 2018Show all

8 papers · 1 filter

astro-ph.GA2018★ 30 cited

The Gaia-ESO Survey: the N/O abundance ratio in the Milky Way

L. Magrini, F. Vincenzo, S. Randich +31

The abundance ratio N/O is a useful tool to study the interplay of galactic processes, e.g. star formation efficiency, time-scale of infall and outflow loading factor We aim to tra…

astro-ph.IM2018

Revisiting the science case for near-UV spectroscopy with the VLT

C. J. Evans, B. Barbuy, B. Castilho +8

In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at far-blue visible wavelengths for the foreseeable future. Hi…

astro-ph.GA2018★ 54 cited

The Gaia-ESO Survey: the origin and evolution of s-process elements

L. Magrini, L. Spina, S. Randich +45

Several works have found an increase of the abundances of the s-process neutron-capture elements in the youngest Galactic stellar populations, giving important constraints to stell…

astro-ph.SR2018★ 42 cited

The Gaia-ESO Survey: properties of newly discovered Li-rich giants

R. Smiljanic, E. Franciosini, A. Bragaglia +41

We report 20 new lithium-rich giants discovered within the Gaia-ESO Survey, including the first Li-rich giant with evolutionary stage confirmed by CoRoT data. Atmospheric parameter…

astro-ph.SR2018★ 66 cited

The Gaia-ESO survey: impact of extra-mixing on C- and N-abundances of giant stars

N. Lagarde, C. Reylé, A. C. Robin +30

The GES survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing a determination of the abundances of the key chemical e…

astro-ph.SR2018★ 21 cited

Deep secrets of intermediate-mass giants and supergiants: Models with rotation seem to overestimate mixing effects on the surface abundances of C, N, and Na

R. Smiljanic, P. Donati, A. Bragaglia +2

Recent observational results have demonstrated an increase in the surface Na abundance that correlates with stellar mass for red giants between 2 and 3 Msun. This trend supports ev…