Fig. 11
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Constraints on the accretion rate onto and total extinction towards PDS 70 b (Mp ≈ 2 MJ). For a given geometry (line thickness or colour), possible values of AH α are rightward of the dashed line (minimum extinction as a function of Ṁ) and along the solid curve (implied by our emission model and LH α from Zhou et al. 2021). Results barely depend on the radius fit (Warm is used here).
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