  It has long been known that rotation can have an appreciable impact on
stellar pulsation --- by modifying the usual p and g modes found in the
non-rotating case, and by introducing new classes of mode. However, it's only
relatively recently that advances in numerical simulations and complementary
theoretical treatments have enabled us to model these phenomena in any great
detail. In this talk I'll review highlights in this area (the 'Greatest Hits'),
before considering the flip side (or the 'B-side', for those of us old enough
to remember vinyl records) of the pulsation-rotation interaction: how pulsation
can itself influence internal rotation profiles.
