Fig. 9
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Comparison of the radial profiles of MP Mus (red) and TW Hya (black) at 1.3 mm. The TW Hya data were taken from Macías et al. (2021), and convolved with a 0.08″Gaussian to match the resolution and distance of the MP Mus observations. The inner cavity and two of the known gaps gaps of TW Hya (at 25 and 45 au) are still visible in the case of TW Hya, in contrast with the smooth profile of MP Mus.
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