CAOSP abstracts, Volume: 48, No.: 1, year: 2018

Abstract: We use 3D magnetohydrodynamic CO5BOLD model atmospheres to study the interplay between magnetic fields and convection in the atmospheres of red giant stars. We find that vortex-like structures occur prominently in stars with stronger magnetic fields and lead to alterations of their thermal structures.

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Last update: February 06, 2018