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

Gaia-Sausage-Enceladus: Lithium evolution from early red-giant-branch and main-sequence stars

C. T. Nguyen, G. Cescutti, M. M. Bennedik +3

The combination of data from the Gaia satellite and large ground-based spectroscopic surveys recently lead to a milestone understanding of our Galaxy's formation history, marked by…

astro-ph.SR2025

Unlocking the mystery of Sr synthesis in the early Galaxy through analysis of barium isotopes in very metal-poor stars

T. M. Sitnova, L. Lombardo, L. I. Mashonkina +8

We determine the contributions of the rapid (r) and slow (s) neutron capture processes to the Ba isotope mixture, along with Ba, Eu, and Sr NLTE abundances, in a sample of very met…

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.GA2025

High N/O ratio at high redshift as a result of a strong burst of star formation and differential galactic winds

F. Rizzuti, F. Matteucci, P. Molaro +2

Recent observations by JWST have revealed supersolar N abundances in galaxies at very high redshift. On the other hand, these galaxies show subsolar metallicity. The observe…

astro-ph.GA2025

Explaining the ratio in the Galactic halo: the contribution from shell mergers in primordial massive stars

F. Rizzuti, G. Cescutti, P. Molaro +5

Recent campaigns of observations have provided new measurements of the carbon isotopes in the most metal-poor stars of the Galaxy. These stars are so metal-poor that they could onl…