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We present preliminary results from an ongoing study of the bulges of S0galaxies. We show that in a subsample of 14 barred S0 galaxies, fully half thephotometrically 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; androunder "inner bulges,'' which appear to be hotter systems more like classicalbulges.Comment: 3 pages, 1 figure; to appear in "Penetrating Bars through Masks of  Cosmic Dust: The Hubble Tuning Fork Strikes a New Note," eds. D. Block, K.  Freeman, R. Groess, I. Puerari, and E.K. Block (Dordrecht: Kluwer

Pseudobulges in Barred S0 Galaxies