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The Dependence of Convective Core Overshooting on Stellar Mass: Reality Check and Additional Evidence

  • Authors: Antonio Claret and Guillermo Torres

2019 The Astrophysical Journal 876 134.

  • Provider: AAS Journals

Caption: Figure 11.

Pressure scale height at the edge of the standard convective core as a function of stellar mass. The relation is based on ZAMS models for solar metallicity and ﹩{\alpha }_{\mathrm{MLT}}=1.80﹩.

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