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Fig. 4
Our model spectrum (red) compared to the IUE spectrum of Feige 34 in the range used for fitting the Ni lines and N v doublet. Lines with equivalent width ≳36 mÅ (given in the labels in mÅ) are indicated. The 1259.5 and 1260.5 Å features are due to S ii and Si ii interstellar lines.
This figure is made of several images, please see below:
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