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The Hubble Space Telescope has provided the first clear evidence for weakerwinds of metal-poor massive stars in the Small Magellanic Cloud, confirmingtheoretical predictions of the metallicity dependence of mass-loss rates andwind terminal velocities. For lower luminosity O-type stars however, derivedmass-loss rates are orders of magnitude lower than predicted, and are atpresent unexplained.

UV Spectroscopy of Metal-Poor Massive Stars in the Small Magellanic Cloud