Combining seismology and spectropolarimetry of hot stars
  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. 
Coralie Neiner, Maryline Briquet, St\'ephane Mathis and Pieter   Degroote
astro-ph.SR