Fig. 5
He I IR pEW as a function of the integrated EUV flux at λ ≤ 504 Å (vacuum). The color-coded models correspond to the new series A and B of models as given in Fig. 2. Black crosses represent the previously nonflaring models from Hintz et al. (2019) as given in Table A.1. The region marked by the blue rectangular in the upper panel is enlarged in the lower panel and shows our most quiescent models.
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