Fig. 8
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Mass limits around DR Tau as obtained from the LMIRCam L′ data (solid orange line) using the AMES-DUSTY models and assuming a system age of 3 Myr. The dashed orange line represents the limits obtained using the total intensity IRDIS data assuming the same model and the same system age. The two black dashed lines give the estimated separation of the compact feature.
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