Normalized continuum flux without the stellar photosphere as function of distance from the center along one direction. The figure is constructed from a NIR image of Model 1 at t/t_acc = 0.7 as an example. The general trend is similar for t/t_acc > 0.5 independent of evolutionary models. The normalized continuum is similar for the various evolutionary models for t/t_acc > 0.5. The continuum is shown to arise in the inner few AU region and to fall off very quickly for i < 60°. However, significant contributions from larger radii are expected for relatively high inclination.