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We present an analysis of the Far Ultraviolet Spectroscopic Explorer({\it{FUSE}}) spectra of the little-known southern nova-like BB Doradus. Thespectrum was obtained as part of our Cycle 8 {\it FUSE} survey of highdeclination nova-like stars.  The FUSE spectrum of BB Dor, observed in a high state, is modeled with anaccretion disk with a very low inclination (possibly lower than 10deg).Assuming an average WD mass of 0.8 solar leads to a mass accretion rate of1.E-9 Solar mass/year and a distance of the order of 650 pc, consistent withthe extremely low galactic reddening in its direction. The spectrum presentssome broad and deep silicon and sulfur absorption lines, indicating that theseelements are over-abundant by 3 and 20 times solar, respectively.

Far Ultraviolet Spectroscopic Explorer Spectroscopy of the Nova-like BB Doradus