Simulations of Core Convection in Rotating A‐Type Stars: Differential Rotation and Overshooting
Simulations of Core Convection in Rotating A‐Type Stars: Differential Rotation and Overshooting
We present the results of three-dimensional simulations of core convection within A-type stars of 2 M☉, at a range of rotation rates. We consider the inner 30% by radius of such stars, thereby encompassing the convective core and some of the surrounding radiative envelope. We utilize our anelastic spherical harmonic …