Fig. A.2.
UVES observation of BAT99 12 (blue line). A zoom-in on a promd He I also includes models for T = 20 kK dwarfs (log g = 4.0 [cgs]), which are diluted to 50%, 10%, and 5% (red, green, and pink lines, respectively). The models assume a typical rotation of 100 km s−1. No features corresponding to a late-type massive secondary can be spotted.
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