collaborators

6 papers

astro-ph.SR2026

Modelling s-process chemical clocks: insights from high-precision Kepler data

G. Casali, M. Molero

We present Galactic chemical evolution (GCE) models for the chemical clocks [Zr/Ti] and [Ce/Ti], tracing first- and second-peak s-process nucleosynthesis, and compare them with a h…

astro-ph.IM2026

HRMOS: A High-Resolution Multi-Object Spectrograph for the VLT

Laura Magrini, Thomas Bensby, Sofia Randich +174

This White Paper presents the scientific rationale and instrument concept for HRMOS (High-Resolution Multi-Object Spectrograph), a next-generation instrument proposed for the ESO V…

astro-ph.GA2025

Mapping the Ages of Stars with Chemistry

Carlos Viscasillas Vázquez, Giada Casali, Laura Magrini +11

Chemical clocks, based on age-sensitive stellar abundance ratios, offer a powerful and scalable approach to reconstruct the formation history of the Milky Way. This white paper out…

astro-ph.GA2025

Rubidium Abundances in Cool Giants from High-Resolution H-band Spectra: A New Diagnostic for Galactic Chemical Evolution

Nils Ryde, Jess Kocher, Govind Nandakumar +6

The Galactic Center and inner disk of the Milky Way contain complex stellar populations obscured by heavy dust extinction. To study their chemical composition, high-resolution near…

astro-ph.GA2025

Shaping Galactic Habitability: the impact of stellar migration and gas giants

E. Spitoni, M. Palla, L. Magrini +9

In exoplanet research, the focus is increasingly on identifying Earth analogs, planets similar in density and habitability potential. As the number of rocky exoplanets grows, paral…

astro-ph.GA2025

Europium, we have a problem. Modelling r-process enrichment across Local Group galaxies

Marco Palla, Marta Molero, Donatella Romano +1

Context: Europium (Eu) serves as a crucial tracer to understand the origin of rapid neutron-capture process (r-process) elements. An extensive effort was made in the last decade to…