H–R diagram showing the comparison of the parameters of D2–EB modeled with the WD code and our three different sets of radial velocities obtained with the fit of He ii of FASTWIND templates (red circles), the fit of all K-band features of H05 spectra except for the Brγ/He i blend (black triangles), and the fit of the CNO/He i blend of the H05 spectra (green squares). The last set is also modeled with ELC and parameters are shown with blue asterisks. Evolutionary tracks and isochrones for single stars (Ekström et al. 2012) at Z = 0.014 with rotation are shown. Isochrones from left to right correspond to 3.2, 4, and 5 Myr. All methods yield co-evolutionary components with an age of ~3.2 Myr that appear overluminous for their masses.