Relativistic modeling of compact stars for charged anisotropic matter in a Tolman IV spacetime

In this paper, we studied the behavior of relativistic objects considering Tolman IV form for the gravitational potential Z and a lineal equation of state within the framework of MIT-Bag model for the charged anisotropic matter. A physical analysis of electromagnetic field indicates that is regular in the origin and well behaved. The new obtained solution not admits singularities in the matter, charge density and metric functions. A graphical analysis indicates that the new stellar model satisfy all physical properties expected in a realistic star.