VLTI-GRAVITY measurements of cool evolved stars - II. Pulsation properties and mass-loss process of the Mira star R Car and the red supergiant VX Sgr

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Fig. 11

Same as Fig. 5 but for the synthetic angular diameters computed from snapshots 119 and 122, i.e., for the minimum (red) and maximum (blue) photospheric radius of our AGB model. Compared to the observations (Fig. 5), the H₂O bands show a weaker extension.

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