A non-local turbulent convection model reproduces Cepheid blue loops and fits observations of five Cepheid binaries as well as mixing length theory with ad-hoc overshooting does, without adjusting per-star parameters.
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Implications of a turbulent convection model for classical Cepheids
A non-local turbulent convection model reproduces Cepheid blue loops and fits observations of five Cepheid binaries as well as mixing length theory with ad-hoc overshooting does, without adjusting per-star parameters.