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Fig. 19

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Images of the integrated intensity (in K km s-1) of CO isotopologues (12CO, 13CO, C17O, and 13C18O) from the series of representative models (Table 1) with dusty inner disk present (δdust = 10-5). Models with δgas = 1,10-1,10-2 and 10-3 are shown. The inclination i = 30° and the black dashed lines show the size of the gap (10 < r < 45 AU). The C18O images look similar to the C17O images and thus not shown. 1st row: 12CO 3 − 2. 2nd row: 13CO 3 − 2. 3rd row: C17O 3 − 2. 4th row: 13C18O 3 − 2.

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