activity
20142026
most citedThe Gaia-ESO Survey. Mg-Al anti-correlation in iDR4 globular clusters

150 citations · 1.1k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.GA2026

A More Complex Than Expected Formation History of the Milky Way's Last Major Merger

Hai-Feng Wang, Guan-Yu Wang, Giovanni Carraro +3

The GaiaSausageEnceladus (GSE) structure, widely recognized as the most recent major accretion event experienced by our Galaxy, is traditionally interpreted as the remnant of…

astro-ph.GA2026★ 1 cited

Photometric Identification of Unresolved Binary Stars in Nearby Open Star Clusters

Varvara O. Mikhnevich, Anastasiia Plotnikova, Giovanni Carraro +1

This paper introduces a new method to search for unresolved binary stars in open star clusters. The work aims at improving the approach introduced previously, which employs the (H-…

astro-ph.GA2025

Counting mass with Gaia: Mass Density of stars and stellar remnants in the solar neighborhood

Artem Lutsenko, Giovanni Carraro, Vladimir Korchagin +2

In the light of new full-sky surveys, many attempts of creating a consistent Galactic model were made. The main interest is to estimate the still poorly understood dark matter cont…

astro-ph.SR2024

The Gaia-ESO Survey: Calibrating the lithium-age relation with open clusters and associations. II. Expanded cluster sample and final membership selection

M. L. Gutiérrez Albarrán, D. Montes, H. M. Tabernero +26

The Li abundance observed in pre-main sequence and main sequence late-type stars is strongly age-dependent, but also shows a complex pattern depending on several parameters, such a…

astro-ph.GA2024

Velocity Dispersion of the open cluster NGC 2571 by Radial Velocities and Proper Motions

Maxim V. Kulesh, Aleksandra E. Samirkhanova, Giovanni Carraro +3

We use a Kernel Density Estimator method to evaluate the stellar velocity dispersion in the open cluster NGC 2571. We derive the 3-D velocity dispersion using both proper motions a…

astro-ph.SR2024

Binary origin of blue straggler stars in Galactic star clusters

M. J. Rain, M. S. Pera, G. Perren +5

Building on the recent release of a new \emph{Gaia}-based blue straggler star catalog in Galactic open star clusters (OCs), we explored the properties of these stars in a cluster s…

astro-ph.GA2024

Binary fraction in Galactic star clusters: FSR 866, NGC 1960, and STOCK 2

Lidia Yalyalieva, Alexandr Chemel, Giovanni Carraro +1

The study of binary stars in different astronomical environments offers insights into the dynamical state of the hosting stellar systems. The Binary Fraction in fact plays a crucia…

astro-ph.SR2021★ 32 cited

Gaia-ESO Survey: Role of magnetic activity and starspots on pre-main sequence lithium evolution

E. Franciosini, E. Tognelli, S. Degl'Innocenti +24

Pre-main sequence models with inflated radii are needed to simultaneously reproduce the colour-magnitude diagram and the lithium depletion pattern in young open clusters. We tested…

astro-ph.GA2021★ 55 cited

The Gaia-ESO Survey: Galactic evolution of lithium from iDR6

D. Romano, L. Magrini, S. Randich +31

We exploit the unique characteristics of a sample of open clusters (OCs) and field stars for which high-precision 7Li abundances and stellar parameters are homogeneously derived by…

astro-ph.SR2020★ 35 cited

The Gaia-ESO Survey: Galactic evolution of lithium at high metallicity

S. Randich, L. Pasquini, E. Franciosini +20

Reconstructing the Galactic evolution of lithium (Li) is the main tool used to constrain the source(s) of Li enrichment in the Galaxy. Recent results have suggested a decline in Li…

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.SR2017★ 57 cited

The Gaia-ESO Survey: Galactic evolution of sulphur and zinc

S. Duffau, E. Caffau, L. Sbordone +48

Due to their volatile nature, when sulfur and zinc are observed in external galaxies, their determined abundances represent the gas-phase abundances in the interstellar medium. Thi…

astro-ph.SR2017★ 150 cited

The Gaia-ESO Survey. Mg-Al anti-correlation in iDR4 globular clusters

E. Pancino, the GES collaboration

We use Gaia-ESO Survey iDR4 data to explore the Mg-Al anti-correlation in globular clusters, that were observed as calibrators, as a demonstration of the quality of Gaia-ESO Survey…

astro-ph.GA2017★ 41 cited

The Gaia-ESO Survey: low-alpha element stars in the Galactic Bulge

A. Recio-Blanco, A. Rojas-Arriagada, P. de Laverny +17

We take advantage of the Gaia-ESO Survey iDR4 bulge data to search for abundance anomalies that could shed light on the composite nature of the Milky Way bulge. The alpha-elements…

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.SR2016★ 31 cited

The Gaia-ESO Survey: the inner disk, intermediate-age open cluster Trumpler 23

J. C. Overbeek, E. D. Friel, P. Donati +33

Context: Trumpler 23 is a moderately populated, intermediate-age open cluster within the solar circle at a Rgc ~6 kpc. It is in a crowded field very close to the Galactic plane and…

astro-ph.SR2016★ 65 cited

The Gaia-ESO Survey: calibration strategy

E. Pancino, the Gaia-ESO Survey collaboration

The Gaia-ESO survey (GES) is now in its fifth and last year of observations, and has already produced tens of thousands of high-quality spectra of stars in all Milky Way components…

astro-ph.SR2016★ 64 cited

The Gaia-ESO Survey: A lithium-rotation connection at 5 Myr?

J. Bouvier, A. Lanzafame, L. Venuti +37

We investigate here the lithium content of young low-mass stars in the 5~Myr-old star forming region NGC~2264 and its relationship with rotation. We combine lithium equivalent widt…

astro-ph.SR2016

The Gaia-ESO Survey: Revisiting the Li-rich giant problem

A. R. Casey, G. Ruchti, T. Masseron +48

The discovery of lithium-rich giants contradicts expectations from canonical stellar evolution. Here we report on the serendipitous discovery of 20 Li-rich giants observed during t…

astro-ph.SR2016★ 41 cited

The Gaia-ESO Survey: membership and Initial Mass Function of the Gamma Velorum cluster

L. Prisinzano, F. Damiani, G. Micela +23

Understanding the properties of young open clusters, such as the Initial Mass Function (IMF), star formation history and dynamic evolution, is crucial to obtain reliable theoretica…

astro-ph.SR2015★ 36 cited

The Gaia-ESO Survey: Stellar radii in the young open clusters NGC 2264, NGC 2547 and NGC 2516

R. J. Jackson, R. D. Jeffries, S. Randich +10

Rapidly rotating, low-mass members of eclipsing binary systems have measured radii significantly larger than predicted by standard models. It has been proposed that magnetic activi…

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.GA2015★ 8 cited

Insights into the properties of the Local (Orion) spiral arm. NGC 2302: First results and description of the program

E. Costa, A. Moitinho, M. Radiszc +4

The spiral structure of the Milky Way is highly uncertain and is the subject of much discussion nowadays. We present the first result from a program that determines the properties…

astro-ph.SR2015★ 50 cited

The Gaia-ESO Survey: Discovery of a spatially extended low-mass population in the Vela OB2 association

G. G. Sacco, R. D. Jeffries, S. Randich +28

The nearby (distance~350-400 pc), rich Vela OB2 association, includes Velorum, one of the most massive binaries in the solar neighbourhood and an excellent laboratory for inv…