activity
20132026
most citedFluorine in the Solar neighborhood: No evidence for the neutrino process

41 citations · 187 across the 16 of their papers we have counts for

collaborators
Showing 2024Show all

5 papers · 1 filter

astro-ph.GA2024★ 12 cited

Modelling chemical clocks -- Theoretical evidences of the space and time evolution of [s/alpha] in the Galactic disc with Gaia-ESO survey

Marta Molero, Laura Magrini, Marco Palla +6

Chemical clocks based on [s-process elements/alpha-elements] ratios are widely used to estimate ages of Galactic stellar populations. However, the [s/alpha] vs. age relations are n…

astro-ph.GA2024★ 4 cited

Yields from massive stars in binaries. Chemical evolution of the Milky Way disk

E. Pepe, M. Palla, F. Matteucci +1

A large fraction of massive stars in the Galaxy reside in binary systems and their evolution is different from that of single stars. The yields of massive stars, which are the main…

astro-ph.GA2024★ 24 cited

Mapping radial abundance gradients with Gaia-ESO open clusters: Evidence of recent gas accretion in the Milky Way disk

Marco Palla, Laura Magrini, Emanuele Spitoni +5

Context. Recent evidences from spectroscopic surveys point towards the presence of a metal-poor, young stellar population in the chemical thin disk. In this context, the investigat…

astro-ph.SR2024

The AMBRE Project: Lead abundance in Galactic stars

G. Contursi, P. de Laverny, A. Recio-Blanco +4

The chemical evolution of neutron capture elements in the Milky Way is still a matter of debate. Although more and more studies investigate their chemical behaviour, there is still…

astro-ph.HE2024★ 9 cited

Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution

Finia P. Jost, Marta Molero, Gerard Navó +3

We provide yields from 189 neutrino-driven core-collapse supernova (CCSN) simulations covering zero-age main sequence masses between 11 and 75 solar masses and three different meta…