Complex asteroseismology of the Slowly Pulsating B-type star HD74560
  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, $\ell$. For two of them, found also in spectroscopic data, we are able to derived the empirical values of the complex nonadiabatic parameter $f$. 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 $\beta$ Cephei stars. 
Przemys{\l}aw Walczak, Wojciech Szewczuk, Jadwiga   Daszy\'nska-Daszkiewicz
astro-ph.SR