Fig. 11.
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Average NIR veiling as a function of the system’s inclination with respect to our line of sight. The solid line is the data’s linear fit, and the fitted line’s slope is given in each panel. We do not consider the discrepant targets (TW Hya and V2247 Oph) to fit the data. The NIR veilings tend to be anti-correlated with the system’s inclination, see text.
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