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Fig. 4


Comparison between the rectified FUSE observation of AB 6 (ID:X0150102000, φ = 0.44, blue ragged line) and the composite synthetic spectrum (red dashed line) for the P v λλ 1118,1128 resonance doublet and the C iii multiplet at λ1176. The WR and O models are depcited by a black solid line and green dotted line, respectively. The narrow absorption features originate in the interstellar medium (ISM).

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