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Fig. A.4

image

Median luminosities for [O i] lines as a function of disk mass for flat (hc = 0.1, ψ = 0.1) and flared (hc = 0.2, ψ = 0.2) disks, shown by the solid and the dashed lines respectively. T Tauri disk models are shown in upper panels and Herbig models are presented in the lower panels.

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