  We propose a model for compact stars in low-mass X-ray binaries(LMXBs) namely
KS 1731-260, EXO 1745-248 and 4U 1608-52. Here we investigate the physical
phenomena of a compact star in the LMXBs. Using our model, we have calculated
central density, surface density, mass(M) and red-shift for the above mentioned
compact stars, which is very much consistent with the reported data. We also
obtain the possible equation of state(EOS) of the stars which is physically
acceptable.
