activity
20122017
most citedThe Gaia-ESO Survey: the Galactic Thick to Thin Disc transition

241 citations · 786 across the 13 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2017★ 30 cited

The Gaia-ESO Survey: Dynamical models of flattened, rotating globular clusters

Sarah M. R. Jeffreson, Jason L. Sanders, N. W. Evans +12

We present a family of self-consistent axisymmetric rotating globular cluster models which are fitted to spectroscopic data for NGC 362, NGC 1851, NGC 2808, NGC 4372, NGC 5927 and…

astro-ph.SR2015★ 20 cited

The Gaia-ESO Survey: Catalogue of H emission stars

Gregor Traven, Tomaž Zwitter, Sophie Van Eck +18

We discuss the properties of H emission stars across the sample of 22035 spectra from the Gaia-ESO Survey internal data release, observed with the GIRAFFE instrument and largely…

astro-ph.GA2015★ 18 cited

The Gaia-ESO Survey: N-body modelling of the Gamma Velorum cluster

M. Mapelli, A. Vallenari, R. D. Jeffries +22

The Gaia-ESO Survey has recently unveiled the complex kinematic signature of the Gamma Velorum cluster: this cluster is composed of two kinematically distinct populations (hereafte…

astro-ph.GA2015★ 66 cited

The Gaia-ESO Survey: a quiescent Milky Way with no significant dark/stellar accreted disc

G. R. Ruchti, J. I. Read, S. Feltzing +26

According to our current cosmological model, galaxies like the Milky Way are expected to experience many mergers over their lifetimes. The most massive of the merging galaxies will…

astro-ph.SR2014★ 73 cited

The Gaia-ESO Survey: the most metal-poor stars in the Galactic bulge

L. Howes, M. Asplund, A. R. Casey +39

We present the first results of the EMBLA survey (Extremely Metal-poor BuLge stars with AAOmega), aimed at finding metal-poor stars in the Milky Way bulge, where the oldest stars s…

astro-ph.GA2014★ 129 cited

The Gaia-ESO Survey: the chemical structure of the Galactic discs from the first internal data release

Š. Mikolaitis, V. Hill, A. Recio-Blanco +31

Most high-resolution spectroscopic studies of the Galactic discs were mostly confined to objects in the solar vicinity. Here we aim at enlarging the volume in which individual chem…