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Using high-resolution imaging with the Hubble Space Telescope, we study theLarge Magellanic Cloud HII region N160A and uncover several striking featuresof this complex massive star-forming site. The two compact high excitation HIIblobs (HEBs) A1 and A2 are for the first time resolved and their stellarcontent and morphology is revealed. A1, being of higher excitation, is poweredby a single massive star whose strong wind has created a surrounding bubble. A2harbors several exciting stars enshrouded inside large quantities of dust. Thewhole N160A nebula is energized by three star clusters for which we obtainphotometry and study their color-magnitude diagram. The HII region isparticularly dusty, with extinction values reaching an A_v~2.5 mag in thevisible, and it is separated from the molecular cloud by an outstandingionization front. A previously detected infrared young stellar object is alsoaccurately located with respect to the HII region.

Resolving the compact $\ion{H}{ii}$ regions in N160A with $\vec{HST}$