  In present paper a spherically symmetric stellar configuration has been
analyzed by assuming the matter distribution of the stellar configuration is
anisotropic in nature and compared with the realistic objects, namely, the low
mass X-ray binaries (LMXBs) and X-ray pulsars. The analytic solution has been
obtained by utilizing the dark energy equation of state for the interior
solution corresponding to the Schwarzschild exterior vacuum solution at the
junction interface. Several physical properties like energy conditions,
stability, mass-radius ratio, and surface redshift are described through
mathematical calculations as well as graphical plots. It is found that obtained
mass-radius ration of the compact stars candidates like 4U 1820-30, PSR J
1614-2230, Vela X-1 and Cen X-3 are very much consistent with the observed data
by Gangopadhyay et al. (Mon. Not. R. Astron. Soc. 431, 3216 (2013)). So our
proposed model would be useful in the investigation of the possible clustering
of dark energy.
