a1 Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio, 3, I-35122, Padova, Italy email: firstname.lastname@example.org
An increasing number of photometric observations of multiple stellar populations in Galactic globular clusters is seriously challenging the paradigm of GCs hosting single, simple stellar populations. These multiple populations manifest themselves in a split of different evolutionary sequences as observed in the cluster color-magnitude diagrams. Multiple stellar populations have been identified in Galactic and Magellanic Cloud clusters. In this paper we will summarize the observational scenario.