activity
20102023
most citedThermohaline instability and rotation-induced mixing. I - Low- and intermediate-mass solar metallicity stars up to the end of the AGB

271 citations · 1.7k across the 34 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2022★ 34 cited

A self-consistent dynamical model of the Milky Way disc adjusted to Gaia data

A. C. Robin, O. Bienaymé, J. B. Salomon +6

This paper shows how a self-consistent dynamical model can be obtained by fitting the gravitational potential of the Milky Way to the stellar kinematics and densities from Gaia dat…

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.GA2021★ 31 cited

Deciphering the evolution of the Milky Way discs: Gaia APOGEE Kepler giant stars and the Besançon Galaxy Model

N. Lagarde, C. Reylé, C. Chiappini +13

We investigate the properties of the double sequences of the Milky Way discs visible in the [/Fe] vs [Fe/H] diagram. In the framework of Galactic formation and evolution, we dis…

astro-ph.GA2021★ 58 cited

Abundance-age relations with red clump stars in open clusters

L. Casamiquela, C. Soubiran, P. Jofré +8

Context: Precise chemical abundances coupled with reliable ages are key ingredients to understand the chemical history of our Galaxy. Open Clusters (OCs) are useful for this purpos…

astro-ph.GA2020★ 22 cited

The Blanco DECam Bulge Survey. I. The Survey Description and Early Results

R. Michael Rich, Christian I. Johnson, Michael Young +18

The Blanco Dark Energy Camera (DECam) Bulge survey is a Vera Rubin Observatory (LSST) pathfinder imaging survey, spanning sq. deg. of the Southern Galactic bulge, $-2^\c…

astro-ph.GA2019★ 64 cited

The Gaia-ESO survey: Calibrating a relationship between Age and the [C/N] abundance ratio with open clusters

G. Casali, L. Magrini, E. Tognelli +51

In the era of large high-resolution spectroscopic surveys, high-quality spectra can contribute to our understanding of the Galactic chemical evolution, providing chemical abundance…