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The uploaded files provide a series of stellar evolution tracks with initial masses from 16 to 20 \(M_\odot\). The two sets of tracks compare the evolution of stars evolved on the red supergiant branch with the Kee et al. turbulent pressure driven mass-loss rates to stars that instead use the de Jager mass-loss rates.
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
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| downloads | 15 |

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