  In this paper, we study the stellar structure in terms of alternative theory
of gravity specially by f (R;T) gravity theory. Here, we consider the function
f (R;T) = R+2VT where R is the Ricci scalar, T is the stress-energy momentum
and V is the coupling constant. Using it we developed a stellar model that
briefly explains the isotropic matter distribution within the compact object
filled with perfect fluid. The stability of the model is shown by several
physical and stability conditions. With the accecptibility of our theory, we
were able to collect data for compact stars like PSR-B0943+10, CEN X-3, SMC
X-4, Her X-1 and 4U1538-52 with great accuracy.
