activity
20052026
most citedChromium: NLTE abundances in metal-poor stars and nucleosynthesis in the Galaxy

188 citations · 2.8k across the 79 of their papers we have counts for

collaborators
Showing 2025Show all

8 papers · 1 filter

astro-ph.GA2025

Fluorine Evolution in the Galactic Halo

Valeria Grisoni, Federico Rizzuti, Gabriele Cescutti

The chemical evolution of fluorine is still a matter of debate in Galactic archaeology, especially at low metallicities, where it is particularly challenging to obtain the correspo…

astro-ph.GA2025★ 13 cited

Impact of AGB stars on the chemical evolution of neutron-capture elements

Gabriele Cescutti, Francesca Matteucci

In this paper we discuss the impact of the s-process nucleosynthesis in Asymptotic Giant Branch stars on the enrichment of heavy elements. We review the main steps made on this sub…

astro-ph.GA2025★ 3 cited

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.SR2025★ 12 cited

PARSEC V2.0: Rotating tracks and isochrones for seven addtional metallicities in the range Z=0.0001-0.03

C. T. Nguyen, G. Costa, A. Bressan +10

PARSEC v2.0 rotating stellar tracks were previously presented for six values of metallicity from subsolar to solar values, with initial rotation rates (, defined as t…

astro-ph.GA2025★ 5 cited

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★ 5 cited

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…