3D CO5BOLD simulations show convective overshoot increases the fully mixed mass in DA white dwarfs by up to 2.5 orders of magnitude and shifts the convection onset temperature to 18000-18250 K.
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18-year monitoring finds stable metal line strengths and accretion rates in four of five polluted white dwarfs over hundreds to thousands of diffusion timescales.
citing papers explorer
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Convective Overshoot and Macroscopic Diffusion in Pure-Hydrogen Atmosphere White Dwarfs
3D CO5BOLD simulations show convective overshoot increases the fully mixed mass in DA white dwarfs by up to 2.5 orders of magnitude and shifts the convection onset temperature to 18000-18250 K.
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Spectroscopic Monitoring of Metal Lines in Polluted White Dwarfs
18-year monitoring finds stable metal line strengths and accretion rates in four of five polluted white dwarfs over hundreds to thousands of diffusion timescales.