  We present far-ultraviolet spectra of the Seyfert2 galaxy Mrk533 obtained
with FUSE. These spectra show narrow asymmetrical OVI 1032,1038 emission lines
with stronger wings shortward of the peak wavelength, but the degree of
asymmetry of these wings in velocity is much lower than that of the wings of
the lines of lower ionization. In the combined OVI profile there are marginal
indications of local absorptions in the outflow. The CIII 977 line is seen
weakly with a similar profile, but with very low signal to noise. These FUV
spectra are among the first for a Seyfert of type2, i.e., a purportedly
obscured Seyfert. The HST STIS spectral image of Mrk533 allows delineation of
the various components of the outflow, and we infer that the outflow is
accelerated. We discuss the results in terms of nuclear geometry and
kinematics.
