International audience
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February 2018 (v1)Journal articleUploaded on: December 4, 2022
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April 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
September 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
July 2017 (v1)Journal article
Context. The spatial distribution of elemental abundances in the disc of our Galaxy gives insights both on its assembly process and subsequent evolution, and on the stellar nucleogenesis of the different elements. Gradients can be traced using several types of objects as, for instance, (young and old) stars, open clusters, HII regions,...
Uploaded on: December 4, 2022 -
May 2017 (v1)Journal article
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 harder to find them inside the solar Galactocentric radius, due to the high mortality rate and strong extinction inside this region. NGC 6802 is one of the inner disk...
Uploaded on: December 4, 2022 -
September 2019 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
2022 (v1)Journal article
Context. 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 for large samples of Galactic stars, complementing Gaia astrometry. Among those surveys, the Gaia-ESO Public Spectroscopic Survey, the only one performed on a...
Uploaded on: December 4, 2022 -
2022 (v1)Journal article
Context. The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100 000 stars, including large representative samples of the stellar populations in the Galaxy, and a well-defined sample of 60 (plus 20 archive) open clusters. We provide internally consistent...
Uploaded on: December 3, 2022