activity
19972026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 22.6k across the 247 of their papers we have counts for

collaborators

249 papers

astro-ph.SR2026

Abundance analysis of three new extremely metal-poor stars, including one CEMP-s star

P. François, T. Suda, S. Wanajo +5

We report a detailed abundance analysis of three extremely metal-poor (EMP) stars thanks to spectra obtained with the high-dispersion spectrograph (HDS) at the Subaru telescope. Th…

astro-ph.SR2026

MINCE IV. A detailed analysis of 37 metal-poor and subsolar metallicity stars

L. Sgatti, G. Cescutti, L. Lombardo +13

The project called Measuring at Intermediate metallicity Neutron-Capture Elements (MINCE) primarily focuses on the photospheric abundances of several neutron-capture (NC) elements…

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.GA2026

TOPoS VII. Age-metallicity relation in the Galactic halo and assembly of the Milky Way

P. Bonifacio, Y. Lebreton, I. Koutsouridou +8

One technique for determining stellar ages is to compare the position of a star in the Hertzsprung-Russell diagram to theoretical stellar evolutionary tracks. The sub-giant evoluti…

astro-ph.GA2026

TYC 170-1218-1: A new r-process-enhanced extremely metal-poor star, rich in Th

E. Caffau, P. Bonifacio, L. Sbordone +5

Context . Extremely metal-poor (EMP) stars are formed from gas clouds enriched by one or a few supernova explosions belonging to the first stellar generation and this very limited…