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Fig. D.1.
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Accretion rate Ṁacc as a function of extinction AV reproducing the observed fluxes of the atomic transitions HI Paδ, Paγ, Paβ and Brγ. The curves are derived from the empirical relations between Lacc and LHI of Alcalá et al. (2017). The intersection of the four curves gives the best estimate of Ṁacc and AV towards DG Tau B.
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