Fig. 8.
Normalised observed accretion rate for TWA 3A (solid green) and DQ Tau (solid red), against the simulated phase-folded accretion curves from T1 (dashed blue) and T2 (dashed orange), which have eccentricities similar to the observed systems. We also show the results of the simulations from Muñoz & Lai (2016) for a binary of eccentricity e = 0.5 (black dash-dotted line).
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