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Fig. 2

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Line fluxes for the v2−1 P(4) transition and the v1−0 P(10) transition, comparing vertical escape flux (star symbols) and detailed line radiative transfer (circles) for the Rin model series. Left plot: TTauri disk case with fluorescence. Right plot: Herbig disk case with fluorescence. Left panel: effect of the inclination from the detailed line radiative transfer for a face-on disk as well (i = 0°).

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