Fig. 6
Simulated H-band polarized intensity image of the Andrews et al. (2011) model convolved with a two-component Gaussian PSF with FWHM = 0.183 arcsec for the broad component and FWHM = 0.038 arcsec for the narrow one. The scales are identical to Fig. 2 for comparison. The green cross gives the stellar position and the magenta circle denotes the inner working angle from our observations.
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