A simple kinematic modeling for flattened S0 galaxies

We present mass models for three S0 galaxies with a strong disk component observed almost on edge (NGC 2732, NGC 4111, and NGC 4350). For the analytical representation of the surface-brightness distribution, the method of Multi- Gaussian Expansion, first presented by Monnet et al. (1992: AA overall agreement is reached, except for the innermost region, where additional mass is needed for all three galaxies. We dis- cuss possible applications.