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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 5.

(a) Same as Figure 1 for SZ Cen, with [Fe/H] = −0.25. (b) ﹩{\alpha }_{\mathrm{MLT}}﹩ for both stars restricted to the CB2018 value of ﹩{{\alpha }_{\mathrm{MLT}}}_{\odot }=1.60﹩ (dots), or to a value of 1.80 near our solar-calibrated mixing length (squares). (c) Same as panel (a), adding the constraint from the measured temperature ratio (see text). (d) Same as panel (b), adding the constraint from the measured temperature ratio. (e)–(h) Same as panels (a)–(d), for [Fe/H] = −0.20.

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