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Fig. 10

image

HR diagram showing the model grid that is used to search for a representative stellar model of HD 201433. The models are color-coded according to their χ2 value and shown with thick lines when at least one mode excited (i.e., with a positive work integral) and with thin lines when all modes are damped. The two best-fit models are marked with black circles. The black rectangle indicates the spectroscopic error box (see Table 7 and Sect. 1).

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