Fig. A.11
Results for the β Cephei star SBL653 with frequency spectra, light curves, and an attempt to identify the pulsation mode of f1 = 9.2647d-1; The second frequency takes the value f2 = 13.334d-1. The determined errors are σf1 = 0.0003d-1 and σf2 = 0.0008d-1. The amplitude ratios were calculated for masses from 15 to 16M⊙. All notations and markings are the same as in Fig. A.3.
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