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20242026
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astro-ph.GA2026

Abundances of CNO in candidate young metal-poor stars

Piercarlo Bonifacio, Elisabetta Caffau, Luca Sbordone +6

In this contribution we investigate the CNO abundances in five apparently young evolved stars, with the aim of discriminating between truly young stars and stars that were rejuvena…

astro-ph.GA2025

The Gaia RVS Benchmark Stars. III . Confirmed and New High Radial Velocity Stars From Gaia DR3

Elisabetta Caffau, David Katz, Piercarlo Bonifacio +12

High-velocity stars are interesting targets to unveil the formation of the Milky Way. In fact they can be recently accreted from an infalling dwarf galaxies or they can be the resu…

astro-ph.GA2025

The most metal poor stars

P. Bonifacio, E. Caffau, P. François +1

The most metal-poor stars found in the Galaxy and in nearby galaxies are witnesses of the early evolution of the Universe. In a general picture in which we expect the metallicity t…

astro-ph.GA2025

Young stars discovered in dwarf spheroidal galaxies confirm their recent infall into the Milky way

Francois Hammer, Piercarlo Bonifacio, Elisabetta Caffau +10

Recent observations from the ESA Gaia satellite and with the ESO VLT, have identified the presence of a population of young, 0.5 to 2 Gyr old, stars in the halo and in dwarf sphero…

astro-ph.GA2025

A Sequoia stellar candidate with very high 7Li and 9Be

L. Monaco, E. Caffau, P. Molaro +2

Aims. The metal-poor star BPM 3066 belongs to the retrograde halo and presents unexpectedly strong spectral features of lithium. To gain insight into the origin of this peculiar ab…

astro-ph.GA2024

Chemical Evolution of R-process Elements in Stars (CERES). III. Chemical abundances of neutron capture elements from Ba to Eu

L. Lombardo, C. J. Hansen, F. Rizzuti +11

The chemical abundances of elements such as barium and the lanthanides are essential to understand the nucleosynthesis of heavy elements in the early Universe as well as the contri…