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Table 2:

Comparison of calculated wind parameters derived using CMF and Sobolev line forces.

Star
$\dot M^{\rm Sob}$ $v_\infty^{\rm Sob}$ $\dot M^{\rm CMF}$ $v_\infty^{\rm CMF}$
  [ \ensuremath{\ensuremath{{M}_{\odot}}~{\rm year}^{-1}}] [ \ensuremath{{\rm km~s}^{-1}}] [ \ensuremath{\ensuremath{{M}_{\odot}}~{\rm year}^{-1}}] [ \ensuremath{{\rm km~s}^{-1}}]
First stars
M500-1 $6.3\times10^{-08}$ 2750 $6.1\times10^{-08}$ 4010
M500-2 $4.0\times10^{-07}$ 1930 $2.0\times10^{-07}$ 1310
M500-3 $2.1\times10^{-07}$ 580 $1.4\times10^{-07}$ 790
M500-4 $3.8\times10^{-08}$ 600 $2.8\times10^{-08}$ 620
O stars
HD 24912 $4.4\times10^{-7}$ 2270 $2.3\times10^{-7}$ 2030
HD 37043 $6.2\times10^{-7}$ 2340 $4.1\times10^{-7}$ 2000
HD 47839 $2.2\times10^{-7}$ 3080 $1.0\times10^{-7}$ 2970
HD 54662 $7.9\times10^{-7}$ 2190 $4.1\times10^{-7}$ 2050
HD 93204 $1.3\times10^{-6}$ 2290 $5.9\times10^{-7}$ 2080
HD 149757 $4.7\times10^{-8}$ 2040 $2.9\times10^{-8}$ 1860
HD 203064 $5.7\times10^{-7}$ 2080 $3.8\times10^{-7}$ 1780
HD 209975 $8.4\times10^{-7}$ 2430 $5.5\times10^{-7}$ 1960
Central stars of planetary nebulae
NGC 2392 $3.7\times10^{-8}$ 490 $1.8\times10^{-8}$ 500
NGC 3242 $3.1\times10^{-9}$ 2000 $2.0\times10^{-9}$ 1890
IC 4637 $3.1\times10^{-8}$ 1440 $1.4\times10^{-8}$ 1270
IC 4593 $7.4\times10^{-8}$ 730 $3.8\times10^{-8}$ 660
He 2-108 $9.5\times10^{-8}$ 730 $4.7\times10^{-8}$ 700
IC 418 $9.5\times10^{-8}$ 730 $4.7\times10^{-8}$ 700
Tc 1 $2.8\times10^{-8}$ 870 $1.8\times10^{-8}$ 800
NGC 6826 $1.8\times10^{-7}$ 870 $7.6\times10^{-8}$ 790


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