activity
20042026
most citedThe Gaia-ESO Survey: the Galactic Thick to Thin Disc transition

241 citations · 1.4k across the 23 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2026

Gaia-Sausage-Enceladus: Lithium evolution from early red-giant-branch and main-sequence stars

C. T. Nguyen, G. Cescutti, M. M. Bennedik +3

The combination of data from the Gaia satellite and large ground-based spectroscopic surveys recently lead to a milestone understanding of our Galaxy's formation history, marked by…

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.GA2017★ 45 cited

The Gaia -ESO Survey: Lithium enrichment histories of the Galactic thick and thin disc

Xiaoting. Fu, D. Romano, A. Bragaglia +32

Lithium abundance in most of the warm metal-poor main sequence stars shows a constant plateau (A(Li)~2.2 dex) and then the upper envelope of the lithium vs. metallicity distributio…

astro-ph.GA2017★ 26 cited

The -ESO Survey: the inner disk intermediate-age open cluster NGC 6802

B. Tang, D. Geisler, E. Friel +43

Milky Way open clusters are very diverse in terms of age, chemical composition, and kinematic properties. Intermediate-age and old open clusters are less common, and it is even har…

astro-ph.GA2016★ 40 cited

The Gaia-ESO Survey: the selection function of the Milky Way field stars

E. Stonkute, S. E. Koposov, L. M. Howes +26

The Gaia-ESO Survey was designed to target all major Galactic components (i.e., bulge, thin and thick discs, halo and clusters), with the goal of constraining the chemical and dyna…

astro-ph.GA2015★ 76 cited

The Gaia-ESO Survey: Characterisation of the [alpha/Fe] sequences in the Milky Way discs

G. Kordopatis, R. F. G. Wyse, G. Gilmore +30

We investigate, using the Gaia-ESO Survey internal Data-Release 2, the properties of the double sequence of the Milky Way discs (defined chemically as the high-alpha and low-alpha…

astro-ph.GA2014★ 11 cited

The Gaia-ESO Survey: α-abundances of metal-poor stars

R. Jackson-Jones, P. Jofré, K. Hawkins +21

We performed a detailed study of the ratio of low-α to high-α stars in the Galactic halo as observed by the Gaia-ESO Survey. Using a sample of 381 metal-poor stars from the second…

astro-ph.GA2014★ 241 cited

The Gaia-ESO Survey: the Galactic Thick to Thin Disc transition

A. Recio-Blanco, P. de Laverny, G. Kordopatis +36

(Abridged) We have used the atmospheric parameters, [alpha/Fe] abundances and radial velocities, determined from the Gaia-ESO Survey GIRAFFE spectra of FGK-type stars (iDR1), to pr…

astro-ph.GA2014★ 204 cited

The Gaia-ESO Survey: radial metallicity gradients and age-metallicity relation of stars in the Milky Way disk

M. Bergemann, G. Ruchti, A. Serenelli +42

We study the relationship between age, metallicity, and alpha-enhancement of FGK stars in the Galactic disk. The results are based upon the analysis of high-resolution UVES spectra…

astro-ph.GA2013★ 47 cited

The Gaia-ESO Survey: Abundance ratios in the inner-disk open clusters Trumpler 20, NGC 4815, NGC 6705

L. Magrini, S. Randich, D. Romano +50

Open clusters are key tools to study the spatial distribution of abundances in the disk and their evolution with time. Using the first release of stellar parameters and abundances…