Fig. 11
Logarithmic luminosity of the low-velocity component of the [OI] 630 nm line vs the logarithm of the accretion luminosity of our objects (red filled symbols) and for two samples of classical T Tauri stars (blue empty circles from Rigliaco et al. 2013, green empty symbols from Natta et al. 2014). Downward arrows are upper limits.
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