Fig. 14
The Si iii λ 4552 line profiles computed with ComBiSpeC compared with the line profiles computed with the TIDES code (dots). In this TIDES calculation, the computation is performed using Voigt local line profiles. The ComBiSpeC code uses the same velocity field that is computed with TIDES, but the local line profile is obtained from the non-LTE TLUSTY radiative transfer calculation. Only the profiles computed for the primary star are shown here.
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