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Fig. 10

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Absorption-modified relationship (solid curves) between H α luminosity and accretion rate for the warm- (left panel) and cold-population (right panel) radius fits for the three accretion geometries (rows; see labels). We consider only absorption by the gas,and also show the case of no absorption (dotted curves). Curves are for masses of 2–16 MJ (bottom to top, but with an inversion in MagAcc-Cold at very high ). Horizontal bands are for the luminosity of PDS 70 b (Zhou et al. 2021) and PDS 70 c (Hashimoto et al. 2020). The fit of Ingleby et al. (2013) for CTTSs is also shown (pink dashed line). For reference, one panel shows extinction arrows for AH α = 4 and 8 mag.

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