Fig. 2.
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(a) Hertzprung-Russel diagram and (b) radial profile of the Schwarzschild discriminant, for the six stars we simulated with MUSIC. Symbols indicate the Cepheids we simulated, and the pink shaded area indicates the instability strip for the evolutionary tracks. Shaded regions also highlight the internal convection zones around which our hydrodynamic simulations are centered.
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