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This article has an erratum: [https://doi.org/10.1051/0004-6361/201526535e]


Fig. 17

image

Left: CaII λ3934 line. The purely photospheric model absorption (black) is plotted alongside the normalized ESPaDOnS spectrum (red) and their difference is plotted in blue. The emission component is clearly narrower than the absorption. Right: CIV λ1548 line as observed by IUE showing a clear P Cygni profile.

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