Modelling the chemical evolution of the Milky Way
  In this review I will discuss the comparison between model results and
observational data for the Milky Way, the predictive power of such models as
well as their limits. Such a comparison, known as Galactic archaeology, allows
us to impose constraints on stellar nucleosynthesis and timescales of formation
of the various Galactic components (halo, bulge, thick disk and thin disk).
