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After a brief introduction into the asteroseismic modelling of stars, weprovide a compilation of the current seismic estimates of the core overshootingparameter and of the rotational frequency of single and binary massive stars.These important stellar parameters have meanwhile become available for elevenOB-type stars, among which three spectroscopic pulsating binaries and onemagnetic pulsator. We highlight the potential of ongoing and future analyses ofeclipsing binary pulsators as essential laboraties to test stellar structureand evolution models of single and binary stars.

Asteroseismology of binary stars and a compilation of core overshoot and rotational frequency values of OB stars