  In this work, we construct stellar models ba-\break sed on the complexity
factor as a supplementary condition which allows to close the system of
differential equations arising from the Gravitational Decoupling. The assumed
complexity is a generalization of the one obtained from the well known Tolman
IV solution. We use Tolman IV, Wyman IIa, Durgapal IV and Heintzmann IIa as
seeds solutions. Reported compactness parameters of SMC X-1 and Cen X-3 are
used to study the physical acceptability of the models. Some aspects related to
the density ratio are also discussed.
