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Fig. B.1:

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Comparison of a model with the same disk parameters, changing only the object, that is the continuum, stellar mass, and stellar radius. The model in black is a good fit to the B268 spectrum. Note the difference in scale for the first and second overtone. The used disk parameters are: Ti = 5000 K; p = −0.75; (NH)i = 8.3 × 1025 cm−2; q = −1.5; Ri = 1.1 R*, ; i = 50°; vG = 2 km s−1 ; and 13CO is not included.

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