Fig. F.1.
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Evolutionary tracks from the model of Baraffe et al. (2015) showing the temporal evolution of the luminosity for low-mass stars. Each curve corresponds to a specific mass (in M⊙), as labelled at the end of the tracks. The red star marker represents the primary V2376 Ori, plotted with its age and luminosity, with associated uncertainties. Its luminosity is computed from the SED.
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