  In this work we have studied the bulk properties of compact stellar object
which is largely motivated by the recent work of Potekhin group who studied the
structure and evolution of compact star on the basis of unified EoS of
Brussels-Montreal group. Here we solved ToV equation of state numerically using
three sets of parameter models to compute pressure, baryon density and bulk
modulus etc over a wide range of matter density. The computed values of the
observables like the stellar interior pressure, bulk modulus and baryon density
have been presented as a function of mass density in the tabular form.
Graphical analysis of computed observables and their comparison with reference
data wherever available have been presented as representative cases.
