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We present an analysis of far-ultraviolet (FUV: 130-180 nm) and optical (U,B, and V) data of the stellar and nebular content of the OB associations LH 9,10, and 13 in the Large Magellanic Cloud region N 11. The FUV images from TheUltraviolet Imaging Telescope strongly select the hot O and B stars; over 1900stars were detected in the FUV to a limiting magnitude of m(FUV) = 17 mag. Theresulting FUV photometry combined with optical ground-based data indicate thereare approximately 88 confirmed or candidate O stars in the LH 9, 10, and 13fields alone (in an area of ~ 41 arcmin$^2$), and possibly as many as 170 to240 O-type stars within the entire 40~arcmin-diameter field of view.

Ultraviolet Imaging Telescope Observations of OB Stars in the N 11 Region of the Large Magellanic Cloud