  Asteroseismology and spectropolarimetry have allowed us to progress
significantly in our understanding of the physics of hot stars over the last
decade. It is now possible to combine these two techniques to learn even more
information about hot stars and constrain their models. While only a few
magnetic pulsating hot stars are known as of today and have been studied with
both seismology and spectropolarimetry, new opportunities - in particular
Kepler2 and BRITE - are emerging and will allow us to rapidly obtain new
combined results.
