  We present new yields of 26Al from Wolf--Rayet stellar winds based on
rotating stellar models which account well for numerous observed properties of
massive stars. We study the impacts on the yields of a change of initial mass,
metallicity and initial rotation velocity. We also consider the effects of a
change of mass loss rates during the Wolf--Rayet phase. We show that for
surface rotation velocities during the core H--burning phase matching to the
observed ones, the quantity of 26Al ejected by a star of a given initial mass
and metallicity is roughly doubled when the effects of rotation are taken into
account. The metallicity dependence of the yield is, on the other hand, very
similar to that obtained from non--rotating models. We estimate that at least
about 20% to 50% (e.g. 0.6 --1.4 Msun) of the live 26Al detected in the
Milky--Way originates from Wolf--Rayet stellar winds. We show the importance of
a good knowledge of the present metallicity gradient and star formation rate in
our galaxy for modeling both the variation of the 26Al surface density with the
galactocentric distance and the global contribution of the Wolf--Rayet stellar
winds to the present galactic mass of 26Al.
