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Fig. 1.


Final images for R CrA system obtained from the best SPHERE dataset taken on 2018 June 19 (chosen because it is the best quality observation epoch). Both of these are obtained from a median of the images at all the wavelengths covered by the two instruments. Left panel: final image obtained with IRDIS. Right panel: final images obtained with IFS. Both images have flux scales in such a way to make the presence of the companion clear. In both images there are however hints of the presence of the jet-like structure described in Sect. 4.

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