Fig. 3

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Left panel: azimuthally averaged radial brightness profile from the ALMA image (black dots) and from our model (blue line). Middle panel: radial cut along the major axis of the Qϕ frames (negative radial direction is along the red-shifted semi-major axis, which is nearly coincident with the south-east direction). Right panel: sepectral energy distribution towards PDS 70; black dots correspond to the source’s photometry and the blue line is our prediction.
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