Fig. 5
Impact of ADI processing on the scattered light distribution from an inclined disk. Left column: synthetic scattered light images in the H band obtained from the HD 100546 model by Mulders et al. (2013a). Right column: the same after the ADI analysis performed by pynpoint. The different rows are models with different asymmetry parameters g with the last one being the IRDIS observations. The flux scales are arbitrary.
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