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Fig. 6


Physical parameters of the wind are plotted as a function of ε (left panels) and p (right panels), while using the Soft SED as the ionizing continua. Top panels: for the closest wind point, we plot the logarithm of Rsph | wind in the left panel A as a function of the disk aspect ratio ε and as a function of the accretion index p in the right panel B. This index is held constant at p = 0.01 for the solutions in the left panels and ε = 0.001 is kept constant for those in the right panels. Each blue circle in the figure represents a MHD solution. The logarithm of two other relevant quantities, nH and vobs for the closest wind point, are labelled at each point; these are their maximum possible values within the wind region for a given MHD solution. Bottom panels: the minimum (imin) and the maximum (imax) equatorial angles of the line of sight, within which the wind can be observed, is plotted as a function of ε (left) and of p (right).

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