In this paper, the authors present a new method to extend Pant’ work (see pant D. N.,Astrophys. Space Sci.,215 (1994) 97) to the case of charged fluid spheres. A number of previously known solutions has been rediscovered in the process (see Singh T.et al., Astrophys. Space Sci.,199 (1993) 113, Patino A. and Rago A.,Gen. Rel. Grav.,21 (1989) 637, Whitman P. G. and Burch R. C.,Phys. Rev. D.,24 (1981) 2049, Pant D. N. and Sah A.,Math. Phys.,20 (1979) 2537). Two classes of solutions are obtained and matched at the boundary with the Reissner-Nordstrom metric.