activity
20152017
most citedThe Gaia-ESO Survey: double, triple and quadruple-line spectroscopic binary candidates

69 citations · 87 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201769 cited

The Gaia-ESO Survey: double, triple and quadruple-line spectroscopic binary candidates

T. Merle, S. Van Eck, A. Jorissen +35

The Gaia-ESO Survey (GES) is a large spectroscopic survey that provides a unique opportunity to study the distribution of spectroscopic multiple systems among different populations…

astro-ph.GA2016

The Gaia-ESO survey: Metal-rich bananas in the bulge

Angus A. Williams, N. W. Evans, Matthew Molloy +25

We analyse the kinematics of giant stars in the direction of the Galactic bulge, extracted from the Gaia-ESO survey in the region $-10^\circ \lesssim \ell \lesssim 10^\…

astro-ph.GA2016

The Gaia-ESO Survey: Probes of the inner disk abundance gradient

H. R. Jacobson, E. D. Friel, L. Jilkova +41

The nature of the metallicity gradient inside the solar circle (R_GC < 8 kpc) is poorly understood, but studies of Cepheids and a small sample of open clusters suggest that it stee…

astro-ph.GA2016

Gaia-ESO Survey: Gas dynamics in the Carina Nebula through optical emission lines

F. Damiani, R. Bonito, L. Magrini +28

We present observations from the Gaia-ESO Survey in the lines of H, [N II], [S II] and He I of nebular emission in the central part of the Carina Nebula. We investigate the prop…

astro-ph.SR2016

The Gaia-ESO Survey: Sodium and aluminium abundances in giants and dwarfs - Implications for stellar and Galactic chemical evolution

R. Smiljanic, D. Romano, A. Bragaglia +40

Stellar evolution models predict that internal mixing should cause some sodium overabundance at the surface of red giants more massive than ~ 1.5--2.0 Msun. The surface aluminium a…

astro-ph.GA201518 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…