  We present Far Ultraviolet Spectroscopic Explorer observations of the
magnetic cataclysmic variable V405 Aurigae. Together with four other DQ Her
type binaries, V405 Aur forms a small subclass of intermediate polars which are
likely to evolve into low magnetic field strength polars, similar to AM Her.
Our co-added FUSE spectrum exhibits broad O VI and C III emission-lines as well
as a narrow O VI emission-line component which likely forms near the white
dwarf surface. The O VI 1032/1038 narrow emission line flux ratio is near 2.0
throughout the orbit, indicative of its formation in an optically thin gas.
Radial velocity measurements of the narrow O VI emission-lines restrict any
orbital modulation to a very low amplitude (Kwd = 2.5+/- 0.5 km/s) indicating,
along with other single peaked broad disk emission lines in the UV and optical,
that the binary system is at low inclination.
