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

Hydrodynamical wind on vertically self-gravitating ADAFs in the presence of toroidal magnetic field