  We have conducted a spectroscopic analysis of the far ultraviolet archival
spectra of four symbiotic variables, EG And, AE Ara, CQ Dra and RW Hya. RW Hya
and EG And have never had a recorded outburst while CQ Dra and AE Ara have
outburst histories. We analyze these systems while they are in quiescence in
order to help reveal the physical properties of their hot components via
comparisons of the observations with optically thick accretion disk models and
NLTE model white dwarf photospheres. We have extended the 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. We
re-examine whether or not 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 in which the white dwarf has a surface temperature as low as
$\sim$20,000K. The very small size of the hot component contributing to the
shortest wavelengths of the FUSE spectrum of CQ Dra agrees with an optically
thick and geometrically thin ($\sim$4\% of the WD surface) hot ($\sim
120,000$K) boundary layer. Our analysis of EG And reveals that its hot
component is a hot, bare, low mass white dwarf with a surface temperature of
80-95,000K, with a surface gravity $\log(g)= 7.5$. For AE Ara, we also find
that a low gravity ($\log(g) \sim 6$) hot ($T \sim 130,000$K) WD accounts for
the hot component.
