Przemysław Walczak, Wojciech Szewczuk, Jadwiga Daszyńska-Daszkiewicz
Seismic modeling of the Slowly Pulsating B-type star HD182255 yields strong constraints on the radial orders of the two dominant modes. For these frequencies, we derive also the empirical values of the complex nonadiabatic parameter $f$. These two seismic tools, i.e., pulsational frequencies and the associated values of $f$, allow to test available opacity data, chemical composition and overshooting efficiency.
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http://arxiv.org/abs/1212.4643
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