Table 2: Best fit model parameters for the polar (p), intermediate (i), and disk wind (d). The mass fluxes are assumed to be constant within the indicated $\theta $-ranges and have an error on the order of 20%.
  T0 $T_{\infty }$ $\theta_{\rm min}$ $\theta_{\rm max}$ $v_\infty$ $F_{\rm m}(\theta)$
  [K] [K] [ $\hbox{$^\circ$ }$] [ $\hbox{$^\circ$ }$] [km s-1] [g s-1 cm-2]
p 50 000 10 000 0 45 85 $7.2\times 10^{-2}$
i 50 000 10 000 45 78 45 $1.5\times 10^{-1}$
d 10 000 6000 78 90 35 $5.5\times 10^{-1}$


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