activity
19932025
most citedAbundance Gradients and the Formation of the Milky Way

688 citations · 11.1k across the 212 of their papers we have counts for

collaborators

214 papers

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.GA2023★ 32 cited

Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk

R. da Silva, V. D'Orazi, M. Palla +25

Classical Cepheids (CCs) are solid distance indicators and tracers of young stellar populations. Our aim is to provide iron, oxygen, and sulfur abundances for the largest and most…

astro-ph.GA2023★ 18 cited

Modeling the chemical enrichment history of the Bulge Fossil Fragment Terzan 5

Donatella Romano, Francesco R. Ferraro, Livia Origlia +9

Terzan 5 is a heavily obscured stellar system located in the inner Galaxy. It has been postulated to be a stellar relic, a Bulge Fossil Fragment witnessing the complex history of t…

astro-ph.GA2023★ 13 cited

Time evolution of Ce as traced by APOGEE using giant stars observed with the Kepler, TESS and K2 missions

G. Casali, V. Grisoni, A. Miglio +11

Abundances of s-capture process elements in stars with exquisite asteroseismic, spectroscopic, and astrometric constraints offer a novel opportunity to study stellar evolution, nuc…

astro-ph.GA2023★ 8 cited

Evolution of radioactive elements in the LMC: predictions for future gamma-ray surveys

Arianna Vasini, Francesca Matteucci, Emanuele Spitoni +1

Short-lived radionuclides, such as 26Al and 60Fe, are tracers of star formation. Therefore, their abundances can unravel the recent star formation history of the host galaxy. In vi…

astro-ph.GA2023★ 9 cited

Europium enrichment and hierarchical formation of the Galactic halo

L. Cavallo, G. Cescutti, F. Matteucci

Context. The origin of the large star-to-star variation of the [Eu/Fe] ratios observed in the extremely metal-poor (at [Fe/H]) stars of the Galactic halo is still a matter…