Fig. 6
Accretion luminosity derived from the luminosity of various emission lines, as labeled, using the relations by Alcalá et al. (2017), and assuming AV = 3.5 mag. The blue line is the best-fit accretion luminosity obtained fitting the whole X-shooter spectrum of CIDA 1. The red line is the mean value of Lacc obtained from the luminosity of the emission lines.
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