the local temperature. In this work, we calculate the total bremsstrahlung emission for the matter from the CENBOL region. Also, we quantify the mass outflow rate calculated assuming an annular cylinder at the injection radius which is concentric with the vertical axis. The thickness of the cylinder is considered to be twice the size of a SPH particle. This ensures at least one SPH particle lies within the cylindrical annulus. We identify particles leaving the computational domain as outflow provided they have positive resultant velocity, $v_r > 0$ and $v_z > 0$ and they lie above the disc height at the injection radius. With this, we estimate the mass outflow rate which is defined as $R_{\dot m}={\rm outflow~rate}~({\dot M}_{\rm out})/
{\rm accretion~rate}~(|{\dot M}_{\rm in}|)$ and observe its time evolution. Here, ${\dot M}_{in(out)} = 2 \pi \rho_{\rm inj(out)}
v_{\rm inj(out)} x_{\rm inj(out)}H_{\rm inj(out)}$. In Figure 4, we present the variation of shock location, corresponding bremsstrahlung flux from the post-shock region and mass outflow rate with time. Here, the radiative flux is plotted in arbitrary unit. Assuming a $10 M_{\sun}$ black hole, the overall time evolution of five seconds ($\equiv$ 50600 code time) is shown for representation. The input parameters are $r_{\rm 