Using the 14 galaxies from the Sauron data which were previously mentioned, we have 
constructed a model for the inner regions of a bulge (out to about 1 effective radius).  
The Sauron velocity fields tend to show that mean velocity is symmetric about the center 
of a galaxy.  Because of this feature, we were able to separate different areas into 
regions of constant velocity.  Averaging all of the Sauron data together, we then produced 
a mean velocity model.  The same was also done for velocity dispersion, where the model 
contains annular regions of decreasing dispersion.  To see how well this model worked, we 
took a uniform field of points and generated a velocity for each point.  The combined 
result of mean velocity and dispersion resembles a rotation curve rather well.