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Fig. 10.
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Comparison between the B-, V-, and I-band light curves of V88 (dots) and the predicted light curves (lines) for stellar parameters corresponding to an evolved RRL pulsator of Z = 0.0006, Y = 0.245, with a period consistent with the observed one and M = 0.59 M⊙, log L/L⊙ = 1.87, and Teff = 6650 K.
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