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Stellar evolution models calculated based on PARSEC V1.2S with a range of core overshooting strength. These models were used and presented in Rosenfield et al., 2017, "A NEW APPROACH TO CONVECTIVE CORE OVERSHOOTING: PROBABILISTIC CONSTRAINTS FROM COLOR-MAGNITUDE DIAGRAMS OF LMC CLUSTERS"
| 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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