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Table 2:

Parameters of our best fit models. Uncertainties are: 3 kK (7 kK for SMC-WR1) on temperatures, 0.1 dex on luminosities (0.15 for SMC-WR1), 0.2 dex on $\dot{M}$, 100 km s-1 on $v_{\infty }$, 0.05 on He/H, 30 to 50$\%$ on abundances.

Star
ST T* T_ eff $T_{{\rm eff}}$ LL_ $\log \frac{L}{L_{\odot}}$ R* $\log \dot{M}$ $f_{\infty }$ $\beta$ $v_{\infty }$ He/H X X(C) X(N) X(O)
    [kK] [kK]   $R_{\odot}$ [$M_{\odot }$ yr-1]     [km s-1] # (%) (%) (%) (%)
SMC-WR1 WN3h 65.4 60.5 5.75 5.8 -5.55 0.10a 1.0 1800 0.25 0.50 <0.004 0.12 <0.04
SMC-WR2 WN5h 44.8 42.5 5.50 9.3 -5.85 0.10a 1.0 1000 0.15 0.62 0.005 0.35 -
SMC-WR4 WN6h 43.1 42.0 5.90 16.0 -5.00 0.15b 1.0 1000 0.45 0.35 0.003 0.40 <0.15
a Adopted.
b Derived from $\chi^{2}$ fit, mass loss rate scaled from model closest to minimum ( $f_{\infty}=0.1$).

Source LaTeX | All tables | In the text

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