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Fig. 5
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Half width at half maximum divided by the square root of the stellar mass for the H2 (orange), [O I] NLVC (blue), and BLVC (red) as a function of the sine of the disk inclination. Keplerian models for gas emitted from disk radii of 0.01, 0.05, 0.2, 0.5, 1, 2, and 3.5 au are shown as solid black lines.
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