Fig. 5
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PI distribution in H band, PIobs;H, for FU Ori and V1735 Cyg (Takami et al. 2018), with a pixel scale of 9.5 mas, normalized to the Stokes I flux of the central source. North is up. In each image, the central region is masked as we were not able to make reliable measurement due to the central source being significantly brighter than the extended emission. Features such as spiral arms are labeled (see the text for details).
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