  The energy transfer of W UMa contact binaries and its effects on the
secondary in W UMa contact binaries are investigated. Relations are given
between the mass ratio (q) and the relative energy transfer rates, i.e. U1, the
ratio of the transferred luminosity to the surface luminosity of the primary
and U2, the ratio of the transferred luminosity to the nuclear luminosity of
the secondary. The theoretical curves(U1 vs q and U2 vs q) are derived.
Although these curves can reflect the distribution of U1 vs q and U2 vs q, some
observational systems are significantly deviated from these curves. It is
mainly resulted from the difference in the effective temperatures of the
components in W UMa systems.The radius and the density of the secondary are
related to the relative energy tran-sfer rate U2: the higher is U2, the greater
is the expansion and the lower is the density of the secondaries in W UMa
systems. The temperature difference of W UMa binary components is correlated
with the relative energy transfer rate U1 and decreases with increasing U1.
This might suggest that there is a thermal coupling between two components in W
UMa contact binaries, and that the classif-ication of W UMa contact binaries
into A- or W-types depends on the energy tran-sfer from the primary to the
secondary. The temperature difference of W UMa bin-ary components is poorly
correlated with the mass of the primary. This suggests that the properties of
the common envelope of W UMa contact binaries might not have a significant
effect on the energy transfer between two components.
