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It is now believed that magnetohydrodynamic equilibria can exist in stablystratified stars due to the seminal works of Braithwaite & Spruit (2004) andBraithwaite & Nordlund (2006). What is still not known is whethermagnetohydrodynamic equilibria can exist in a barotropic star, in which stablestratification is not present. It has been conjectured by Reisenegger (2009)that there will likely not exist any magnetohydrodynamical equilibria inbarotropic stars. We aim to test this claim by presenting preliminary MHDsimulations of barotropic stars using the three dimensional stagger code ofNordlund & Galsgaard (1995).

Search for Stable Magnetohydrodynamic Equilibria in Barotropic Stars