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Fig. 9
FLiTs spectra of the disk models from 0.56 Myr old, convolved to a spectral resolution R = 2800 (black lines) and R = 600 (red lines). Where indicated, the spectra were multiplied by 5, 10, or 50 in order to improve visibility. This disk is at an inclination of 45°. The y-axis limits are different than those in Fig. 8.
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