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Table 10:

Assumed abundances used in computing the wind absorption model.
Parameter Adopted value Explanation
$X_{{\rm H}}^{{\rm WR}}$ 0.44 H percentage in massf
$X_{{\rm He}}^{{\rm WR}}$ 0.55 He percentage in mass
$X_{{\rm C}}^{{\rm WR}}$ $3.0 \times 10^{-4}$ C percentage in mass
$X_{{\rm N}}^{{\rm WR}}$ $1.0 \times 10^{-2}$ N percentage in mass
$X_{{\rm O}}^{{\rm WR}}$ $3.0 \times 10^{-3}$ O percentage in mass
$X_{{\rm Ne}}^{{\rm WR}}$ $1.75\times 10^{-3}$ Ne percentage in mass
$X_{{\rm Mg}}^{{\rm WR}}$ $6.53 \times 10^{-4}$ Mg percentage in mass
$X_{{\rm Si}}^{{\rm WR}}$ $7.02 \times 10^{-4}$ Si percentage in mass
$X_{{\rm S}}^{{\rm WR}}$ $3.67 \times 10^{-4}$ S percentage in mass
$X_{{\rm Fe}}^{{\rm WR}}$ $1.84 \times 10^{-3}$ Fe percentage in mass
$X_{{\rm H}}^{{\rm O}}$ 0.71 Hydrogen percentage in mass
    (solar abundances adoptedg)

f Crowther et al. (1995a); g Anders & Grevesse (1989).

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