Fig. 4
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HST/STIS spectrum of the O(He) star JL 9 compared to the final model spectrum (red graph; Teff = 80 000 K, logg = 5.2) with the element abundances given in Table 4. The same model attenuated by interstellar lines is plotted in blue. Prominent photospheric lines are identified. Question marks indicate unidentified lines. A reddening of EB-V = 0.06 was applied to the model spectra.
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