collaborators

6 papers

astro-ph.SR2026

Beryllium enhancement in stars of the accreted Thamnos-2 system

Paolo Molaro, Piercarlo Bonifacio, Elisabetta Caffau +2

Surveys of Galactic halo stars have revealed numerous streams and substructures tracing stellar populations accreted by the Milky Way. Among these, Gaia-Sausage-Enceladus (GSE) and…

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.SR2025

The chemical DNA of the Magellanic Clouds V. R-process dominates neutron capture elements production in the oldest SMC stars

Lorenzo Santarelli, Marco Palla, Alessio Mucciarelli +4

We present the chemical abundances of Fe, alpha- and neutron-capture elements in 12 metal-poor Small Magellanic Cloud (SMC) giant stars, observed with the high-resolution spectrogr…

astro-ph.SR2025

Fast Rotating Blue Straggler Stars in the globular cluster NGC 1851

Alex Billi, Lorenzo Monaco, Francesco R. Ferraro +4

In this work we study the rotational velocities of a sample of blue straggler stars (BSSs) and reference stars belonging to the Galactic globular cluster NGC 1851, using high-resol…

astro-ph.SR2025

The chemical DNA of the Magellanic Clouds III. The first, extragalactic Mg-K anticorrelation: the LMC globular cluster NGC 1786

Deimer Antonio Alvarez Garay, Alessio Mucciarelli, Lorenzo Monaco

In this work we derived [K/Fe] and [Mg/Fe] abundance ratios for six stars of the old globular cluster NGC 1786 in the Large Magellanic Cloud. We employed high-resolution spectra ac…

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…