  We present the effect of a hydrodynamical wind on the structure and the
surface temperature of a vertically self-gravitating magnetized ADAFs using
self-similar solutions. Also a model for an axisymmetric, steady-state,
vertically self-gravitating hot accretion flow threaded by a toroidal magnetic
field has been formulated. The model is based on $\alpha-$prescription for
turbulence viscosity. It is found that the thickness and radial velocity of the
disc are reduced significantly as wind gets stronger. In particular, the
solutions indicated that the wind and advection have the same effects on the
structure of the disc. We also find that in the optically thin ADAF becomes
hotter by including the wind parameter and the self-gravity parameter.

High Energy Astrophysical Phenomena