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Fig. A.1
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The differences of the Tx values as computed by Eq. (1) for the two selected band widths (legend) relative to the one used in this work (6.2–41.3 Å), assuming CIE. Symbols belong to the PN bubbles of the 0.696 M⊙ simulation. The evolution of Tx occurs from low to high values and back when the star fades (cf. Fig. 13).
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