Fig. 15
Line fluxes per unit surface as a function of the accretion luminosity. The meaning of the symbols is as in Fig. 10. The value of the rank-correlation coefficient ρ is also reported in each box. The subluminous objects were excluded because Lacc is underestimated (Alcalá et al. 2014, 2017), while the surface fluxes are not affected. Downward arrows indicate upper limits.
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