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We present the results of complex seismic modelling of the Slowly PulsatingB-type star HD74560. The star pulsates in five frequencies detected inphotometric observations. For all these frequencies, we identify the modedegree, $\ell$. For two of them, found also in spectroscopic data, we are ableto derived the empirical values of the complex nonadiabatic parameter $f$. Wetest effects of chemical composition and opacity data. Our results show thatthe properties of seismic models of SPB stars differ significantly from thoseof the more massive $\beta$ Cephei stars.

Complex asteroseismology of the Slowly Pulsating B-type star HD74560