Stellar models with like-Tolman IV complexity factor

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