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Fig. 3


MFs derived for IRDIS data in BB-J (right) and BB-K (left) in F0 (shown in Fig. 1, top). Last three red bins represent the MF considering the A1 and C as a binaries and B as a single source. The last three black stars represent the MF if the WR stars are considered single objects, which is the case for the photometry analysis.

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