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Fig. 15.
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Evolution of the mode frequency ν1, 11, norm along an avoided crossing taking place at central densities between ρc = 13 000 and 18 000 g.cm−3 for the models of the stellar subgrid with fov = 0.00. The transition mass, between radiative and convective cores in the MS, is 1.182 M⊙ for this choice of fov.
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