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Fig. 6


Wind lines of NGC 346-031. A comparison of our best-fit model (blue line) with a model computed using the parameters provided in Mokiem et al. (2006) (red line). The mass-loss rates differ by almost two orders of magnitude. The blue side of N vλ1240 is affected by interstellar Ly α absorption. We also show the Hα line, which proves to be insensitive to mass-loss over a wide range of values.

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