collaborators

5 papers

astro-ph.SR2026

Wide binaries without viable bound Newtonian orbits

L. Pasquini, R. Saglia, F. Patat +7

Context. Wide binaries offer a unique opportunity to test gravity in the low acceleration regime, where deviations from Newtonian dynamics may appear. Aims. We use high-resolution…

astro-ph.GA2026

Evidence for multiple crossings and stripping of Gaia-Enceladus/Sausage across the Milky Way

L. Berni, M. Palla, L. Magrini +1

The accretion of Gaia-Enceladus/Sausage (GES) onto the Milky Way (MW) is one of the most prominent features of the Galactic halo revealed by the combination of the Gaia satellite a…

astro-ph.IM2025

Tracing the Early Milky Way with Globular Clusters: The Diagnostic Power of Neutron-Capture Elements

J. Schiappacasse-Ulloa, L. Berni, S. Lucatello +3

Globular clusters (GCs) are fundamental tracers of the early assembly of the Milky Way (MW). They formed in diverse environments -- including both our Galaxy and dwarf galaxies --…

astro-ph.GA2025

Exploring substructures in the Milky Way halo Neural networks applied to Gaia and APOGEE DR 17

L. Berni, L. Spina, L. Magrini +3

The identification of stellar structures in the Galactic halo, including stellar streams and merger remnants, often relies on the dynamics of their constituent stars. However, this…

astro-ph.GA2025

Neutron-Capture Element Signatures in Globular Clusters: Insights from the Gaia-ESO Survey

J. Schiappacasse-Ulloa, L. Magrini, S. Lucatello +8

Globular clusters (GCs) are key to understanding the formation and evolution of our Galaxy. While the abundances of light and Fe-peak elements in GCs have been widely studied, inve…