Fig. 14
O–C plots for variables V14 and V28 showing the quadratic fit to the time dependence of the difference between observed and predicted times of light curve maxima. The values found using this quadratic fit for V14 and V28 are consistent with those derived using our grid fitting method (see text), β = + 1.553 d Myr-1 (V14) and β = + 0.102 d Myr-1 (V28).
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