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

12 citations · 17 across the 6 of their papers we have counts for

collaborators

12 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.GA20263 cited

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.GA2025

The Milky Way in motion: gauging stellar trajectories that shape the Galactic thin disc

M. L. L. Dantas, R. Smiljanic, R. S. de Souza +2

As stars traverse the Milky Way, their orbits evolve through perturbations that alter their orbital radii. These changes arise from two mechanisms: churning, which modifies angular…

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

Lithium evolution in the Galactic thin disc from Main-Sequence and early Red-Giant-Branch stars

C. T. Nguyen, G. Cescutti, F. Matteucci +7

The role of novae as producers of galactic lithium has been suggested since the 1970s, and it has been reconsidered recently with the detection of Be in their outbursts. At the…

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…