We investigate stellar metallicity distribution functions (MDFs), including Fe and α-element
abundances, in dwarf galaxies from the Feedback in Realistic Environment (FIRE) project …

We present metallicity distribution functions (MDFs) for the central regions of eight dwarf
satellite galaxies of the Milky Way: Fornax, Leo I and II, Sculptor, Sextans, Draco, Canes …

We present detailed chemical abundances for 99 red-giant branch stars in the centre of the
Sculptor dwarf spheroidal galaxy, which have been obtained from high-resolution …

We derive the star formation histories of eight dwarf spheroidal (dSph) Milky Way satellite
galaxies from their alpha element abundance patterns. Nearly 3000 stars from our …

We use the OMEGA galactic chemical evolution code to investigate how the assumptions
used for the treatment of galactic inflows and outflows impact numerical predictions. The …

We investigate the nature of the newly discovered Ultra Faint dwarf spheroidal galaxies (UF
dSphs) in a general cosmological context simultaneously accounting for various …

We investigate the chemical properties of local galaxies within a cosmological framework in
the hierarchical picture of galaxy formation. To this aim, we use a hierarchical semi-analytic …

We propose a cosmological scenario for the formation and evolution of dwarf spheroidal
galaxies (dSphs), satellites of the Milky Way (MW). An improved version of the semi …

We present alpha to iron abundance ratios for 226 individual red giant branch stars in nine
dwarf galaxies of the Andromeda (M31) satellite system. The abundances are measured …

Context. Dwarf spheroidal (dSph) galaxies are the least luminous, least massive galaxies
known. Recently, the number of observed galaxies in this class has greatly increased thanks …