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Imagine we could do asteroseismology of large samples of OB-type stars byusing just one spectrum per target. That would be great! But this is probably acrazy and stupid idea. Or maybe not. Maybe we have the possibility to open anew window to investigate stellar oscillations in massive stars that has beenin front of us for many years, but has not attracted very much our attention:the characterization and understanding of the so-called macroturbulentbroadening in OB-type stars.

Asteroseismology of OB stars with hundreds of single snapshot spectra (and a few time-series of selected targets)