collaborators

17 papers

astro-ph.SR2026

Intrinsic iron abundance spreads in globular clusters

J. Schiappacasse-Ulloa, S. Lucatello, L. Magrini +2

Globular Clusters (GCs) host multiple stellar populations, likely composed of a subset of FG stars that enriched the intracluster medium and gave rise to SG stars, each characteris…

astro-ph.SR2026

Observational Signatures and Constraints on the Intermediate Neutron-Capture Process. The Case of the CEMP star TYC 6044-714-1 (RAVE J094921.8-161722)

Riano E. Giribaldi, Diego Vescovi, Laura Magrini +6

Observational abundances of CEMP stars with patterns in between those produced by the rapid and slow nucleosynthesis processes (CEMP-rs stars) are currently invoked as evidence of…

astro-ph.SR2026

The nucleosynthesis of Ba in the Early Universe. Constraints from elemental abundances and isotopic ratios

Riano E. Giribaldi, Marco Palla, Laura Magrini +6

The [Ba/Eu] abundance ratio is commonly adopted as a tracer of the relative contributions of the slow (s) and rapid (r) neutron-capture processes. However, at [Fe/H] < -2 dex, Ba c…

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.SR2026

Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample

H. Ramler, S. P. D. Borthakur, C. P. Folsom +16

The characterisation of exoplanetary systems depends on the accurate determination of host star parameters. The Ariel mission will probe the atmospheres of a statistically signific…

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…