Tomography of cool giant and supergiant star atmospheres - I. Validation of the method

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Fig. 2

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FWHM of the CFLD_DI for lines contributing to spectral masks C1–C7 (C8 not represented, see text) computed from the 1D-RSG model of Table 1. The color-code identifies the masks as in the middle panel of Fig. 1.

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