Abstract
We report the characterisation of star cluster complexes in the dIrr galaxy NGC 1427A, presently infalling towards the core of the Fornax galaxy cluster, likely for the first time. Using the spatial resolution of HST/ACS and auxiliary VLT/FORS ground-based observations, we study the properties of the most recent episodes of star formation in this gas-rich galaxy, the only one of its type near the core of the Fornax cluster.
