Fig. 4
Solidlines: mean radial profile of the non-deconvolved SPHERE and VISIR images of WR104. All profiles are shifted for readability reasons. Dotted lines: radial profiles of the PSF reference star. The diamonds indicate the theoretical angular resolution of the 8 m telescope at the given wavelength. We also show the position of the companion B star of WR104 (vertical line) for information (see Sect. 5.3).
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