Image Details
Caption: Figure 2.
Hertzsprung–Russell diagram of κ Tuc (top) and ξ Sco (bottom) based on the data of Table 1. The magenta and red lines are PARSEC isochrones (Bressan et al. 2012) for solar metallicity and ages of 1 and 2 Gyr, respectively. Asterisks on the isochrones mark the adopted masses of the components.
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