  Aims: In the present work we search for a new model of compact star within
embedding class one spacetime i.e., four dimensional spacetime embedded in five
dimensional Pseudo Euclidean space.
  Methods: In particular we propose a new mass function to obtain an exact
analytic solutions of the Einstein field equations. For this specific? mass
function, obtained solutions are well-behaved at the centre of the star,
satisfy all energy conditions and the mass-radius relation fall within the
limit proposed by Buchdahl [1].
  Results: The static equilibrium condition has been maintained under different
forces. We have discussed the solutions in detail and compare with a set of
astrophysical objects like 4U1608-52, PSR J1903+327, PSR J1614-2230 and X-ray
pulsar Vela X-1 is also explored.
