activity
20042022
most citedDynamical age differences among coeval star clusters as revealed by blue stragglers

216 citations · 1.3k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2022★ 133 cited

The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products

G. Gilmore, S. Randich, C. C. Worley +165

The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100,000 stars, including large representat…

astro-ph.GA2022★ 188 cited

The Gaia-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacy

S. Randich, G. Gilmore, L. Magrini +161

In the last 15 years different ground-based spectroscopic surveys have been started (and completed) with the general aim of delivering stellar parameters and elemental abundances f…

astro-ph.SR2019★ 69 cited

The extended halo of NGC 2682 (M 67) from Gaia DR2

R. Carrera, M. Pasquato, A. Vallenari +8

Context: NGC 2682 is a nearby open cluster, approximately 3.5 Gyr old. Dynamically, most open clusters should dissolve on shorter timescales, of ~ 1 Gyr. Having survived until now,…

astro-ph.GA2018★ 104 cited

Expanding associations in the Vela-Puppis region: 3D structure and kinematics of the young population

T. Cantat-Gaudin, C. Jordi, N. J. Wright +9

The Vela-Puppis region is known to host the Vela OB2 association as well as several young clusters featuring OB and pre-main sequence stars. Several spatial and kinematic subgroups…

astro-ph.SR2018★ 56 cited

A ring in a shell: the large-scale 6D structure of the Vela OB2 complex

T. Cantat-Gaudin, M. Mapelli, L. Balaguer-Núñez +3

The Vela OB2 association is a group of 10 Myr stars exhibiting a complex spatial and kinematic substructure. The all-sky Gaia DR2 catalogue contains proper motions, parallaxes (a p…

astro-ph.SR2017★ 36 cited

The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon I

G. G. Sacco, L. Spina, S. Randich +44

The young (~2 Myr) cluster Chamaeleon I is one of the closest laboratories to study the early stages of star cluster dynamics in a low-density environment. We studied its structura…