  This paper is devoted to study the analytic models of anisotropic compact
stars in $f(T)$ gravity (where $T$ is torsion scalar), with non-diagonal
tetrad. By taking the anisotropic source inside the spherically symmetric star,
the equations of motions have been derived in the context of $f(T)$ gravity.
Krori and Barua metric which satisfies the physical requirement of a realistic
star, has been applied to describe the compact objects like strange stars. We
use the power law form of $f(T)$ model to determine explicit relations of
matter variables. Further, we have found the anisotropic behavior, energy
conditions, stability and surface redshift of stars. Using the masses and radii
of 4$U$1820-30, Her X-1, SAX J 1808-3658, we have determined the constants
involved in metric components. Finally we discuss the graphical behavior of the
analytic description of strange star candiddates.
