I will present an overview of the potential impact of radial migration on the chemical evolution of the Milky Way disk, based on the results of N-body simulations and semi-analytical models. I will discuss, in particular, the impact on local observables (the local age-metallicity relation and its dispersion, the local metallicity distribution etc.), as well as the chemical properties of the thin and thick disks. I will also present new results obtained with recent yields of rotating massive stars for all elements from C to Pb.

References
Kubryk, Prantzos and Athanassoula (2013) MNRAS
Kubryk, Prantzos and Athanassoula (2015a,b) A&A
Prantzos, Abia, Limongi, Chieffi, Cristallo (2018), A&A in press