  NGC 602 is a young stellar cluster located in a peripheral region of the
Small Magellanic Cloud known as the wing. Far from the main body of the galaxy
and abutting the Magellanic Bridge, the SMC's wing is characterized by low gas
and stellar content. With deep optical imaging from the Advanced Camera for
Surveys (ACS) aboard the Hubble Space Telescope (HST), we have discovered an
extensive pre-Main Sequence (PMS) population, with stellar masses in the range
0.6-3 Solar masses. These low mass PMS stars formed coevally with the central
cluster about 4 Myr ago. Spitzer Space Telescope (Spitzer) images of the same
region from the Infrared Array Camera (IRAC) also reveal a population of Young
Stellar Objects (YSOs), some of which are still embedded in nebular material
and most of which likely formed even more recently than the young stars
detected with HST/ACS imaging. We infer that star formation started in this
region about 4 Myr ago with the formation of the central cluster and gradually
propagated towards the outskirts where star formation is presently ongoing.
