  This paper deals with existence of strange stars in $f\left(T\right) $
modified gravity. For this purpose, we have taken the diagonal tetrad field of
static spacetime with charged anisotropic fluid and MIT bag model, which
provide the linear relation between radial pressure and density of the matter.
Further, the analysis of the resulting equations have been done by assuming the
parametric form of the metric functions in term of the radial profiles with
some unknown constant (introduced by Krori and Barua). By the matching of two
metrices, unknown constant of the metric functions appear in terms of mass,
radius and charge of the stars, the observed values of these quantities have
been used for the detail analysis of the the derived model. We have discuss the
regularity, anisotropy, energy conditions, stability and surface redshift of
the model.
