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Fig. 13

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Closure phase residuals of L-band models (different versions of model 3) with different inner rim parameters ε and Rε as a function of the central star scaling factor. The best-fit models are those two with ϵ = 0.6 and Rϵ = 1.8 and 2.2 Rin at the central star scaling factor 8.4.

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