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Fig. 9


Comparison of parameters for stars in common with Repolust et al. (2004) and Markova et al. (2014), FASTWIND studies (top) and Martins et al. (2015a) – CMFGEN (bottom). Open symbols indicate stars for which we have detected clear or likely signatures of spectroscopic binarity. The dashed line is the 1:1 relation and each panel shows the mean and standard deviation of differences.

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