collaborators

7 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.EP2026

The small transiting planet population revealed by ESPRESSO with extreme precision radial velocities

M. J. Hobson, B. Lavie, F. Bouchy +35

Small planets are extremely common in the Galaxy, including planets with masses and radii between those of Earth and Neptune. Characterizing these planets' masses requires ultra-pr…

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

Unveiling the nature of HE 0107-5240

E. Caffau, M. Steffen, P. Molaro +27

The vast majority of the most iron-poor stars in the Galaxy exhibit a strong carbon enhancement, with C/H ratios only about two orders of magnitude below solar. This unusual chemic…

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.HE2025

Possible evidence for the 478 keV emission line from Be decay during the outburst phases of V1369 Cen

L. Izzo, T. Siegert, P. Jean +4

After decades of uncertainty about the origin of lithium, recent evidence suggests Galactic novae as its main astrophysical source. In this work, we present possible evidence for t…