Improvements to stellar structure models, based on a grid of 3D convection simulations - II. Calibrating the mixing-length formulation
We perform a calibration of the mixing length of convection in stellar structure models against realistic 3D radiation-coupled hydrodynamics simulations of convection in stellar surface layers, determining the adiabat deep in convective stellar envelopes.
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Trampedach_Improvements_to_stellar_2014.pdf||4.43 MB||Adobe PDF|
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