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Fig. 5

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Comparison between models (red dash-dotted and blue dashed lines) and observed (black full line) spectra of HD53138. The red model includes neither clumping nor X-rays in the wind and illustrates the current status in the literature regarding the UV spectral fitting of cool BSGs. The blue model includes clumping (fv,∞= 0.1) but no X-rays.

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