Fig. B.2.
Separations and flux ratios of PDS 37 when modelled as binary. The best fit binary models (a, b, c) are presented in Fig. 1. All binary models indicate separations of ∼22–28 mas which correspond to 42–54 au at the distance of the source. The flux ratios are characterized by a large uncertainty but we observe decreasing flux ratios with increasing separations.
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