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Fig. 28


(Teff, log  g)-representation for the 50 candidate hybrid stars and 1 evolved δ Scuti star. We show the location of the objects belonging to the classes S, P(+VAR), CMP, and SB, as well as the rapidly rotating stars (FAST). The empirical borders of the classical δ Scuti (in black) and γ Dor (in colour) instability strips are represented by solid lines.

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