Simulations of Core Convection in Rotating A-Type Stars: Magnetic Dynamo Action

@article{Brun2005SimulationsOC,
  title={Simulations of Core Convection in Rotating A-Type Stars: Magnetic Dynamo Action},
  author={Allan Sacha Brun and Matthew Keith Morris Browning and J. Toomre},
  journal={The Astrophysical Journal},
  year={2005},
  volume={629},
  pages={461-481}
}
Core convection and dynamo activity deep within rotating A-type stars of 2 M☉ are studied with three-dimensional nonlinear simulations. Our modeling considers the inner 30% by radius of such stars, thus capturing within a spherical domain the convective core and a modest portion of the surrounding radiative envelope. The magnetohydrodynamic (MHD) equations are solved using the anelastic spherical harmonic (ASH) code to examine turbulent flows and magnetic fields, both of which exhibit intricate… 
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