Fig. 9
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Result of RDI Elias 2-24. Significant emission is noticeable in the inner regions of the disk compared to the gap observed by ALMA (green contours). The position of “b” indicated in the image refers to the candidate of Jorquera et al. (2021). The two blobs visible to the west of the star are remnants of the PSF that were not correctly subtracted during the RDI.
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