  We present preliminary results from an ongoing study of the bulges of S0
galaxies. We show that in a subsample of 14 barred S0 galaxies, fully half the
photometrically defined bulges show kinematic signatures of "pseudobulges" --
that is, their kinematics are dominated by rotation. In four of these galaxies,
we identify at least two subcomponents in the photometric bulge region:
flatter, disk or bar components, assocated with disklike kinematics; and
rounder "inner bulges,'' which appear to be hotter systems more like classical
bulges.
