  In the present article, we have constructed static anisotropic compact star
models of Einstein field equations for the spherical symmetric metric of
embedding class one. By assuming the particular form of metric function $\nu$,
We have solved the Einstein field equations for anisotropic matter
distribution. The anisotropic models are representing the realistic compact
objects such as SAX J 1808.4-3658 (SS1), Her X - 1, Vela X-12, PSR J1614-2230
and Cen X - 3. We have reported our results in details for compact star Her X-1
on the ground of physical properties such as pressure, density, velocity of
sound, energy conditions, TOV equation and red-shift etc. Along with these, we
have also discussed about stability of the compact star models. Finally we made
the comparison between our anisotropic stars with the realistic objects on the
key aspects as central density, central pressure, compactness and surface
red-shift.
