Fig. 12.
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Probability density functions and their correlations obtained by MCMC of the power spectrum of 16 Cyg B and for coefficients a1, a2, a3, and a4 for 16 Cyg B. The red curve shows the expected 
coefficient for a pure centrifugal distortion of the star. The light and dark grey PDF fillings are the 1σ and 2σ confidence intervals, respectively.
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