Table 4: The best-fit model parameters for the outflowing wind model. Most parameters are self-explanatory (see Appendix A for details). C1 is the ratio between the polar and equatorial mass flux; m1 is the exponent of the mass flux law as a function of latitude; m2 is the exponent of the latitude dependent terminal velocity law.
Photospheric density $1\pm0.5\times10^{12}~\text{cm}^{-3}$
Equatorial rotational velocity $400\pm50~\ensuremath{\text{km~s}^{-1}} $
Polar terminal velocity $600\pm50~\ensuremath{\text{km~s}^{-1}} $
Terminal velocity above disk $70\pm20~\ensuremath{\text{km~s}^{-1}} $
Polar mass flux $3.2\pm0.2\times10^{-9}~\ensuremath{\ensuremath{M_\odot}~\ensuremath{\text{yr}}^{-1}} $
C1 $0.25\pm0.05$
m1 $30\pm10$
m2 $10\pm2$
Inclination angle (i) $25\pm5\ensuremath{^{\circ}} $

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