Fig. 13.
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Comparison between the PW relation(s) calculated in this paper for the fundamental F-mode δ Sct (as in Fig. 12) and those of F- (red dots) and the first overtone 1O-mode (blue dots) classical Cepheids. For the latter pulsators, the data and the PWs were taken from Poggio et al. (2021). For clarity, only objects with relative error on the photometric parallax better than 20% are plotted.
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