Seismic models of O and B stars with Kurucz’s opacity data

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Fig. A.2

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Same as Fig. A.1, but the Rosseland-mean opacities lgκ_R [ cm² g^-1 ] calculated by Castelli & Kurucz for enhanced abundances of O, Ne, Mg, Si, S, Ar, Ca, and Ti elements by +0.4 dex, viz., opacity data Nos. 23–35 listed in Table A.1 were plotted.

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