Current State of MHD Simulation of Massive Star Winds

In magnetic massive stars, the competition between highly non-linear radiative forces and magnetic field leads to a highly 
complex interaction. Such an interplay cannot usually be modeled analytically, instead numerical modeling become a 
necessary tool. In  this talk, I will discuss how numerical magnetohydrodynamic (MHD) simulations are employed to 
understand the nature of such magnetized massive star winds. I will also briefly outline  the challenges involved in such 
simulations, especially in 3D.