activity
19972026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 28.3k across the 161 of their papers we have counts for

collaborators
Showing 2021Show all

8 papers · 1 filter

astro-ph.SR2021★ 43 cited

The Gaia-ESO Survey: Target selection of open cluster stars

A. Bragaglia, E. Alfaro, E. Flaccomio +36

The Gaia-ESO Survey (GES) is a public, high-resolution spectroscopic survey with FLAMES@VLT. GES targeted in particular a large sample of open clusters (OCs) of all ages. The diffe…

astro-ph.GA2021★ 18 cited

Stellar Population Astrophysics (SPA) with the TNG: Stock 2, a little-studied open cluster with an eMSTO

J. Alonso-Santiago, A. Frasca, G. Catanzaro +14

Stock 2 is a little-studied open cluster that shows an extended main-sequence turnoff (eMSTO). In order to investigate this phenomenon and characterise the cluster itself we perfor…

astro-ph.SR2021★ 58 cited

Chemical evidence for planetary ingestion in a quarter of Sun-like stars

Lorenzo Spina, Parth Sharma, Jorge Meléndez +5

Stellar members of binary systems are formed from the same material, therefore they should be chemically identical. However, recent high-precision studies have unveiled chemical di…

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.GA2021★ 30 cited

Stellar Population Astrophysics (SPA) with TNG Atmospheric parameters of members of 16 unstudied open clusters

R. Zhang, S. Lucatello, A. Bragaglia +12

Thanks to modern understanding of stellar evolution, we can accurately measure the age of Open Clusters (OCs). Given their position, they are ideal tracers of the Galactic disc. Ga…

astro-ph.SR2021★ 54 cited

The Gaia-ESO survey: Mixing processes in low-mass stars traced by lithium abundance in cluster and field stars

L. Magrini, N. Lagarde, C. Charbonnel +42

We aim to constrain the mixing processes in low-mass stars by investigating the behaviour of the Li surface abundance after the main sequence. We take advantage of the data from th…