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Fig. 4

image

Masses (total mass of the pair A and B) as derived from the analysis of period changes with respect to the inclination of the 2.9 yr orbit. The red solid lines represent the masses reported by Lee et al. (2008), the blue lines stand for the masses from our analysis (with the grey area showing the uncertainties). The black line represents the different masses with respect to the inclination between the orbits.

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