We have used the full radial extent of images from the Hubble Space Telescope's Advanced Camera for Surveys and Wide Field Planetary Camera 2 to extract surface brightness profiles from a sample of six, local lenticular galaxy candidates. We have modelled these profiles using a core-Sérsic bulge plus an exponential disk model. Our lenticular disk galaxies with bulge magnitudes M V −21.30 mag have central stellar deficits, suggesting that these bulges may have formed from 'dry' merger events involving supermassive black holes while their surrounding disk was subsequently built up, perhaps via cold gas accretion scenarios. The central stellar mass deficits M def are roughly 0.5 to 2 M BH (black hole mass), rather than ∼10 to 20 M BH as claimed from some past studies, which is in accord with core-Sérsic model mass deficit measurements in elliptical galaxies. Furthermore, these bulges have Sérsic indices n ∼ 3, half light radii R e < 2 kpc and masses > 10 11 M ⊙ , and therefore appear to be descendants of the compact galaxies reported at z ∼ 1.5 to 2. Past studies which have searched for these local counterparts by using single-component galaxy models to provide the z ∼ 0 size comparisons have over-looked these dense, compact and massive bulges in today's early-type disk galaxies. This evolutionary scenario not only accounts for what are today generally old bulges-which must be present in z ∼ 1.5 images-residing in what are generally young disks, but it eliminates the uncomfortable suggestion of a factor of 3 to 5 growth in size for the compact, z ∼ 1.5 galaxies that are known to possess infant disks.
