  We have carried out a spectroscopic analysis of the far ultraviolet spectra
of six symbiotic variables. Two systems, LT Del, which has had one recorded
outburst, and BD-21 3873 (= IV Vir) which has had no recorded outburst, are
yellow symbiotic systems. Two other systems, V443 Her and RW Hya, have also
never had a recorded outburst. Two other symbiotics, StHa190 and CQ Dra, are
more strongly interacting with an outburst history. We have studied these
systems during their quiescence in order to shed light on the nature of their
hot components by fitting their archival far ultraviolet spectra with optically
thick accretion disk models and NLTE model white dwarf photospheres. Using the
critical advantage offered by extending wavelength coverage down to the Lyman
Limit with FUSE spectra, we find that the hot component in RW Hya is a low mass
white dwarf with a surface temperature of 160,000K while the symbiotic system
CQ Dra is a triple system with a red giant transferring matter to a hot
component made up of a cataclysmic variable whose white dwarf has a surface
temperature of $\sim$50,000K. Implications are discussed.
