We present high spatial resolution HST imaging of the LMC compact HII region
N159-5. This high excitation blob is revealed to be a papillon' or butterfly-shaped ionized nebula with the wings’ separated by ~2.3" (0.6 pc).
Two subarcsecond features resembling a smoke ring' and a globule’ are
detected in the wings, the origin of which is briefly discussed. N159-5 may
represent a new type of HII region in the Magellanic Clouds overlooked so far
because of insufficient spatial resolution. Our images also show a strikingly
turbulent medium around the Papillon in the giant HII region N159, which
manifests itself by a large number of subarcsecond filaments, arcs, ridges, and
fronts carved in the ionized gas by the stellar winds from massive stars in the
N159 complex.

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