This article has 2 errata:
[https://doi.org/10.1051/tpe/2021006]
[https://doi.org/10.1051/0004-6361/202038534e]
Fig. 8
Half-width at half maximum divided by the square root of the stellar mass for the H2 (top) and [O I] (bottom) NLVC as a function of the sine of the disk inclination. Keplerian models for gas emitted from disk radii of 0.05, 0.50, 1.00, 2.00, 6.00, and 20.00 au are shown as solid red lines. Bottom panel: empty circles refer to stars whose H2 profile is not detected.
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