  Zero age main sequence models of uniformly rotating stars have been computed
for ten masses between 1.625 and 8 M_\odot and 21 rotation rates from zero to
nearly critical rotation. The surface shape is used to distinguish rotation
rather than the surface equatorial velocity or the rotation rate. Using the
surface shape is close to, but not quite equivalent to using the ratio of the
rotation rate to the critical rotation rate. Using constant shape as the
rotation variable means that it and the mass are separable, something that is
not true for either the rotation rate or surface equatorial velocity. Thus a
number of properties, including the ratio of the effective temperature anywhere
on the surface to the equatorial temperature, are nearly independent of the
mass of the model, as long as the rotation rate changes in such a way to keep
the surface shape constant.
