Fig. B.1
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Line-to-continuum flux ratio, characteristic size, and photocentre shift of the MA II model at five different azimuth angles from −90° to +90°. The inclination of the image is fixed at 20° to conform to the observational value obtained from VLTI GRAVITY data for the inner disk of RU Lup in 2021. The images depict the emission region at 0 km/s.
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