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Table 2:

Final ``best-fit'' values of the model parameters of the stars in the HD 5980 binary system for $i = 86^{\circ }$ and prior to the 1994 LBV outburst.
  Primary eclipse Secondary eclipse
  Ingress Ingress & Egress
star A $\rho_1 = 0.158 \pm 0.005$
    $L_1 = 0.398 \pm 0.021$
star B $\rho_3 = 0.108 \pm 0.003$
  $\rho_2 = 0.269 \pm 0.014$
  $L_{2} = 0.300 \pm 0.016$    
  $y = 0.19 \pm 0.02$
  $u_{2} = 0.58 \pm 0.07$ $v = 0.52 \pm 0.14$

Source LaTeX | All tables | In the text

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