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Fig. 8


Mass accretion rate for FU Tau A derived from various emission line fluxes and luminosities and from the 10% width of Hα using different calibrations provided in the literature as labeled in the figure. Dashed and dotted lines represent the mean and standard deviation for the relations from Alcalá (in prep.) using 20 emission lines as described in Sect. 5.2.1.

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