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Table 3:

Initial mass estimate (in solar units) from evolutionary diagrams. The second and third column give estimates based respectively on the X(H)-L and HR diagram. The errors take into account uncertainties on T_ eff $T_{{\rm eff}}$ and LL_ $\log \frac{L}{L_{\odot}}$. Tracks with $Z = 0.2~Z_{\odot}$ from Meynet & Maeder (2005) are used.
Star X(H)-L T_ eff $T_{{\rm eff}}$ - L

$\rm 34.4^{+10.1}_{-7.8}$ >40

$\rm 22.8^{+5.4}_{-5.8}$ $\rm 47.3^{+7.0}_{-10.6}$
4 $\rm 42.2^{+6.9}_{-7.8}$ $\rm 64.7^{+16.0}_{-10.1}$

Source LaTeX | All tables | In the text

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