  This paper presents an exact solution of the Einstein-Maxwell field equations
in a static and spherically symmetric Schwarzschild canonical coordinate system
in the presence of charged perfect fluid. We have employed the Vaidya-Tikekar
ansatz for the metric potential. Using graphical analysis and tabular
information we have shown that our model obeys all the physical requirements
and stability conditions required for a realistic stellar model. This
theoretical model approximates observations of pulsar PSR B0943+10 to an
excellent degree of accuracy.
