  In a survey of the UV-brightest AGN using the Far Ultraviolet Spectroscopic
Explorer (FUSE), we commonly find associated absorption in the O VI 1032,1038
resonance doublet. Of 34 Type I AGN observed to date with z < 0.15, 16 show
detectable O VI absorption. Most absorption systems show multiple components
with intrinsic widths of ~100 km/s spread over a blue-shifted velocity range of
less than 1000 km/s. With the exception of three galaxies (Ton S180, Mrk 478,
and Mrk 279), those galaxies in our sample with existing X-ray or longer
wavelength UV observations also show C IV absorption and evidence of a soft
X-ray warm absorber. In some cases, a UV absorption component has physical
properties similar to the X-ray absorbing gas, but in others there is no clear
physical correspondence between the UV and X-ray absorbing components.
