252 citations · 3.3k across the 91 of their papers we have counts for
7 papers · 2 filters
Fluorine in the Solar Neighborhood: Chemical Evolution Models
E. Spitoni, F. Matteucci, H. Jönsson +2
In the light of the new observational data related to fluorine abundances in the solar neighborhood stars, we present here chemical evolution models testing different fluorine nucl…
Origin of the Galactic Halo: accretion vs. in situ formation
E. Spitoni, F. Vincenzo, F. Matteucci +1
We test the hypothesis that the classical and ultra-faint dwarf spheroidal satellites of the our Galaxy have been the building blocks of the Galactic halo by comparing their [O/Fe]…
The AMBRE Project: chemical evolution models for the Milky Way thick and thin discs
V. Grisoni, E. Spitoni, F. Matteucci +5
We study the chemical evolution of the thick and thin discs of the Galaxy by comparing detailed chemical evolution models with recent data from the AMBRE Project. The data suggest…
The chemical evolution of the Milky Way
Francesca Matteucci, Emanuele Spitoni, Donatella Romano +1
We will discuss some highlights concerning the chemical evolution of our Galaxy, the Milky Way. First we will describe the main ingredients necessary to build a model for the chemi…
The connection between the Galactic halo and ancient Dwarf Satellites
E. Spitoni, F. Vincenzo, F. Matteucci +1
We explore the hypothesis that the classical and ultra-faint dwarf spheroidal satellites of the Milky Way have been the building blocks of the Galactic halo by comparing their [O/F…
The Galactic habitable zone around M and FGK stars with chemical evolution models with dust
E. Spitoni, L. Gioannini, F. Matteucci
The Galactic habitable zone is defined as the region with highly enough metallicity to form planetary systems in which Earth-like planets could be born and might be capable of sust…