The central main belt is dynamically limited in semi-major axis by the 3J:-1A and 5J;-2A mean-motion resonances  (Zappalá et al. 1995).   The linear secular resonance g-g₆ separates the low-inclined asteroid region from the highly inclined area, dominated by the Hansa and Pallas families (Carruba 2010b).  As discussed in Carruba (2010b), in the highly inclined region the local web of linear secular resonances and mean-motion resonances divided the region into six separated stable islands, each hosting one or more major families, and that can be considered as a stable archipelago.  Of particular interest in this region is the Tina family, whose members are all in anti-aligned states of the g-g₆ linear secular resonance (Carruba and Morbidelli 2011).  We found 3693 objects that have proper elements and frequencies, SDSS-MOC4 a* and i-z colors, WISE geometric albedo data, and satisfy our error analysis criteria, in the central main belt.  The central main belt is a transitional region, where CX-complex and S-complex asteroids are rather mixed.  A greater proportion of S-type asteroids can be found at lower semi-major axis (and vice-versa), but overall, no group dominate the local taxonomy.