Relative Importance of Convective Uncertainties in Massive Stars
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Inlist used for the paper: "Relative Importance of Convective Uncertainties in Massive Stars" (arXiv:2006.01877) The stellar tracks and profile outputs are available on http://www.astro.keele.ac.uk/shyne/datasets/convective-boundary-mixing-uncertainties This work was done with MESA version 10398.
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Zenodo创建时间：
2020-06-05
