FUSE Observations of Variability in Hot-Star Winds
  New constraints on the large-scale wind structures responsible for discrete absorption components are obtained from far-ultraviolet time-series observations of O supergiants in the Large Magellanic Cloud. 
A. W. Fullerton, D. L. Massa, R. K. Prinja, I. D. Howarth, A. J.   Willis, & S. P. Owocki