  The present paper is devoted to investigate the possible emergence of
relativistic compact stellar objects through modified $f(R,T)$ gravity. For
anisotropic matter distribution, we used Krori and Barura solutions and two
notable and viable $f(R,T)$ gravity formulations. By choosing particular
observational data, we determine the values of constant in solutions for three
relativistic compact star candidates. We have presented some physical behavior
of these relativistic compact stellar objects and some aspects like energy
density, radial as well as transverse pressure, their evolution, stability,
measure of anisotropy and energy conditions.
