Considering the full spectrum of linear unstable modes allows the turbulent diffusion coefficient in thermohaline convection to self-consistently interpolate between previously discrepant theoretical scalings.
M., Garaud, P., & Stellmach, S
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MIST provides a new publicly available grid of solar-scaled stellar isochrones and evolutionary tracks computed self-consistently with MESA from pre-main sequence through advanced stages for masses 0.1-300 solar masses and metallicities -2 to 0.5.
MESA Star has been substantially updated with new capabilities for low-mass giant planets, asteroseismology coupling, rotating star models, and uninterrupted massive star evolution to core collapse.
citing papers explorer
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Unifying Transport Models of Thermohaline Convection in Stars
Considering the full spectrum of linear unstable modes allows the turbulent diffusion coefficient in thermohaline convection to self-consistently interpolate between previously discrepant theoretical scalings.
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MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
MIST provides a new publicly available grid of solar-scaled stellar isochrones and evolutionary tracks computed self-consistently with MESA from pre-main sequence through advanced stages for masses 0.1-300 solar masses and metallicities -2 to 0.5.
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Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
MESA Star has been substantially updated with new capabilities for low-mass giant planets, asteroseismology coupling, rotating star models, and uninterrupted massive star evolution to core collapse.