Open Access

Fig. B.4


Simulated low resolution (R = 30) MATISSE visibilities based on the model combining the best-fit continuum model from Sect. 3.2.3, with a C-CH disk component from Sect. 4.4. Different inner radii of the C-CH disk with a flat intensity profile are explored – see the legend on the left hand side, the inner radius of the second. The telescope pairs, projected baseline length (B) and the position angles of the projected baseline (BPA) are shown in each subplot.

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