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Fig. 2

image

Examples of the comparison between the RV data of the primary star and relations 1 and 2 with the best-fit parameters given in Col. (4) of Table 1. The top panels correspond to data from Struve (1944, and Hill et al. (1974, . The bottom panels show one epoch of IUE data from Stickland et al. (1997, and one epoch of FEROS data presented by Sana et al. (2008a) and reanalysed here (right).

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