  We have proposed a model for relativistic compact star with anisotropy and
analytically obtained exact spherically symmetric solutions describing the
interior of the dense star admitting non-static conformal symmetry. Several
features of the solutions including drawbacks of the model have been explored
and discussed. For this purpose we have provided the energy conditions,
TOV-equations and other physical requirements and thus thoroughly investigated
stability, mass-radius relation and surface redshift of the model. It is
observed that most of the features are well matched with the compact stars,
like quark/strange stars.
