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We present examples of an extended asteroseismic modelling in which we aim atfitting not only pulsational frequencies but also certain complex parameterrelated to each frequency. This kind of studies, called \textbf{complexasteroseismology}, has been successfully applied to a few main sequence B-typepulsators and provided, in particular, plausible constraints on \textbf{stellaropacities}. Here, we briefly describe our results for three early B-type stars.

Complex asteroseismology of the B-type main sequence pulsators