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Fig. 6.
Ultra-violet spectra of the models of the Z = 1/5 Z⊙ series for which a spectral type O4V((f)) or O5V((f)) was attributed (see Table A.1). The HST/COS spectrum of the O4−5V star AzV 388 in the SMC, from Bouret et al. (2013), is inserted in red. The main lines are indicated. The initial masses of the models are also given.
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