Table 6: WR line strengths, observed/predicted in the dereddened CAHA spectrum.
Quantity  L(He II $\lambda $4686) N III $\lambda $4640/He II $\lambda $4686
  (1035 erg s-1)  
Observed 3.0 $\pm$ 0.2 0.17 $\pm$ 0.01
Model 13 $\pm$ 9 0.2 $\pm$ 0.1


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