Fig. 8
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Side by side comparison between the observations and a RADMC-3D model with CAHP-128-100nm grains, plus residuals. Left to right: data, model, residuals. Rows (top to bottom): K-band total intensity, Stokes Q, and Stokes U. We did not model the ALMA images using CAHP grains as we do not have the optical properties of the CAHP grains at millimetre wavelengths.
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