  The Magellanic Clouds offer a unique variety of star forming regions seen as
bright nebulae of ionized gas, related to bright young stellar associations.
Nowadays, observations with the high resolving efficiency of the Hubble Space
Telescope allow the detection of the faintest infant stars, and a more complete
picture of clustered star formation in our dwarf neighbors has emerged. I
present results from our studies of the Magellanic Clouds, with emphasis in the
young low-mass pre-main sequence populations. Our data include imaging with the
Advanced Camera for Surveys of the association LH~95 in the Large Magellanic
Cloud, the deepest observations ever taken with HST of this galaxy. I discuss
our findings in terms of the Initial Mass Function, which we constructed with
an unprecedented completeness down to the sub-solar regime, as the outcome of
star formation in the low-metallicity environment of the LMC.
