Abstract
We present the results of complex seismic modelling of the Slowly Pulsating B-type star HD74560. The star pulsates in five frequencies detected in photometric observations. For all these frequencies, we identify the mode degree, . For two of them, found also in spectroscopic data, we are able to derived the empirical values of the complex nonadiabatic parameter . We test effects of chemical composition and opacity data. Our results show that the properties of seismic models of SPB stars differ significantly from those of the more massive Cephei stars.
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