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This article has 2 errata:
[https://doi.org/10.1051/tpe/2021006]
[https://doi.org/10.1051/0004-6361/202038534e]
Fig. 9
Rk(H2)∕Rk([O I]NLV) plotted against Rk(H2). Rk is the disk radius where the H2 or [O I]NLV component originates, under the assumption of Keplerian motion.
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