As in this Paper I present the results for stellar models which differ
from previous papers of this series essentially in the chemical
composition the description of the physics input will be not
repeated here.
The main characteristics and the justification for the stellar models
presented
are described in Claret 1995 (Paper I).
Besides the difference in the initial chemical composition, I also compute
the
tidal constants E2 and the tidal coefficients 
for a few
models of
these grids. In the next papers of this series these calculations will be
available
for all models. Meanwhile I can provide specific calculations under
request.
Such parameters are very important in order to evaluate the critical times
for
circularization and synchronization in close binary systems (CBS) (see
Claret & Cunha 1996).