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Fig. 4


K-band MCFOST modeling of visibility (top) and closure phase in degrees (bottom) for various values of model parameters. Left: various stellar luminosities are compared: 22 L (green), 26 L (red), and 32 L (blue). Middle: effect of the field-of-view when using the AT (red) or UT (black) telescopes. With the latter, only the inner disk of HD 100546 is seen, which is shown in green. The black and green curves lie on top of each other, as expected. Right: the interferometric observables are plotted for different locations of the inner edge of the outer disk, Rin,2 =  9 AU (blue), 13 AU (red), and 17 AU (green).

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