  In this paper, we study magnetized winds described by variable adiabatic
index equation of state in Paczy\'{n}ski \& Wiita pseudo-Newtonian potential.
We identify the flow solutions with the parameter space of the flow. We also
confirm that the physical wind solution is the one which passes through the
slow, Alfv\'en and fast critical points. We study the dependence of the wind
solution on the Bernoulli parameter $E$ and the total angular momentum $L$. The
adiabatic index, which is a function of temperature and composition, was found
to be variable in all the outflow solutions. For the same values of the
Bernoulli parameter and the total angular momentum, a wind in strong gravity is
more accelerated, compared to a wind in Newtonian gravity. We show that flow
variables like the radial and azimuthal velocity components, temperature all
depend on the composition of the flow. Unlike the outflow solutions in
hydrodynamic regime, the terminal speed of a magnetically driven wind also
depends on the composition parameter.
