  In the present study we search for a new stellar model with spherically
symmetric matter and charged distribution under general relativistic framework.
The model represents a compact star of embedding class one. The solutions
obtain here are general in their nature having the following two features:
firstly, the metric becomes flat and also the expressions for the pressure,
energy density and electric charge become zero in all the cases if we consider
the constant $A=0$, which shows that our solutions represent the so-called
`electromagnetic mass model' \cite{Lorentz1904}, and secondly, the metric
function $\nu(r)$, for the limit $n$ tends to infinity, converts to
$\nu(r)=C{r}^{2}+ ln~B$, which is the same as considered by Maurya et al.
\cite{Maurya2015a}. We have investigated several physical aspects of the model
and find that all the features are acceptable within the demand of the
contemporary theoretical studies and observational evidences.
