Fig. 9.
Hertzsprung–Russell diagram for the five M-type stars found within 10′ from the location of HIP 79124 A. The BHAC15 isochrones (Baraffe et al. 2015) are used to estimate their age. We also include the closest A0-type star and confront it against the Dartmouth standard models (Dotter et al. 2008). The inner and the outer figures share axes.
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