In recent years a number of authors have found solutions to the Einstein-Maxwell field equations for static gravitational fields with isotropic matter. These solutions may be utilized to model a charged relativistic star as they are matchable to the Reissner-Nordstrom exterior at the boundary. It is for this reason that many investigators use a variety of techniques to attain exact solutions. This book provides exact solutions to the isotropic Einstein-Maxwell system that model the interior of relativistic stars. The field equations are transformed to simpler forms; the integration of the...