Table 3: Stars with H $_{\rm\alpha }$ in absorption: Errors in stellar and wind parameters given in Table 1. Notation and units as in Table 2, except for the adopted uncertainty in $\beta $ and the corresponding uncertainty in ${\dot M}$ (for stellar radii from Table 1, see text). The upper and lower limits of ${\dot M}$ (in units of $10^{-6}~{M_{\odot}/\rm yr}$) correspond to the lower and upper limits of $\beta $, respectively. The listed errors in $T_{\rm eff}$ and $\log Q_2$ (cf. Table 2) have to be preceeded by a $\pm $sign.
Star $\Delta $ $T_{\rm eff}$ $\Delta $ $\beta $ ${\dot M}$-1 ${\dot M}$+1 $\Delta $ $\log Q_2$ $\Delta $ $\log Q_t$
HD 93128 1.5 $\rm ^{+0.15}_{-0.15}$ 1.59 3.70 0.023 $\rm ^{+0.15}_{-0.22}$
HD 93250 1.5 $\rm ^{+0.10}_{-0.10}$ 2.58 3.87 0.023 $\rm ^{+0.05}_{-0.13}$
HD 303308 1.5 $\rm ^{+0.20}_{-0.10}$ 1.35 2.00 0.027 $\rm ^{+0.09}_{-0.09}$
HD 15558 1.5 $\rm ^{+0.20}_{-0.10}$ 3.84 6.31 0.027 $\rm ^{+0.06}_{-0.16}$
HD 193682 1.5 $\rm ^{+0.20}_{-0.10}$ 0.94 2.16 0.028 $\rm ^{+0.10}_{-0.27}$
HD 15629 1.0 $\rm ^{+0.20}_{-0.10}$ 0.85 1.55 0.018 $\rm ^{+0.08}_{-0.18}$
HD 190864 1.0 $\rm ^{+0.20}_{-0.10}$ 0.97 1.85 0.020 $\rm ^{+0.13}_{-0.16}$
HD 193514 1.5 $\rm ^{+0.20}_{-0.10}$ 2.90 4.16 0.033 $\rm ^{+0.08}_{-0.09}$
HD 24912 1.0 $\rm ^{+0.20}_{-0.10}$ 0.74 1.29 0.022 $\rm ^{+0.08}_{-0.17}$
HD 203064 1.0 $\rm ^{+0.20}_{-0.10}$ 0.94 1.77 0.022 $\rm ^{+0.10}_{-0.18}$
HD 217086 1.0 $\rm ^{+0.20}_{-0.10}$ $\le$0.05 $\le$0.33 0.021 $\rm ^{+0.17}_{-0.68}$
HD 13268 1.0 $\rm ^{+0.20}_{-0.10}$ $\le$0.12 $\le$0.34 0.024 $\rm ^{+0.13}_{-0.33}$
HD 207198 1.0 $\rm ^{+0.20}_{-0.10}$ 1.29 2.33 0.024 $\rm ^{+0.12}_{-0.14}$
HD 209975 1.0 $\rm ^{+0.20}_{-0.10}$ 1.55 2.28 0.025 $\rm ^{+0.04}_{-0.14}$
HD 18409 1.5 $\rm ^{+0.15}_{-0.15}$ 0.74 1.54 0.040 $\rm ^{+0.18}_{-0.14}$
HD 191423 1.0 $\rm ^{+0.20}_{-0.10}$ $\le$0.28 $\le$0.46 0.024 $\rm ^{+0.06}_{-0.17}$
HD 149757 1.0 $\rm ^{+0.20}_{-0.10}$ $\le$0.04 $\le$0.25 0.024 $\rm ^{+0.14}_{-0.65}$


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