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Fig. 1


HR-diagram showing our stellar evolutionary tracks with LMC metallicity. Each dot indicates a stellar model color-coded according to the highest ratio of turbulent-to-total pressure encountered within the stellar model (see color bar on the right). The numbers close to the tracks indicate the zero-age main-sequence mass of the models. Models with between 10% and 33% are shown in red. The absolute maximum is found for the massive red supergiants.

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