Probing planet formation and disk substructures in the inner disk of Herbig Ae stars with CO rovibrational emission

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Fig. D.1

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COemitting radius versus the near-infrared excess flux as fraction of the total stellar flux. Black circles show the inner model radius against the near-infrared excess for the fiducial, g/d = 100, model (see Sect. 4 for details). The data are shown following the same color coding as in Fig. 1.

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