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Fig. 4
Comparison between the best-fit models of the UV spectrum (red lines) and models with higher mass-loss rates (blue lines). The solid lines are the observed spectra. The left panel shows the comparison for HD 46150, the right panel for HD 46202. The narrow absorption features in the C iv 1548–1550 profiles are interstellar.
This figure is made of several images, please see below:
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