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Caption: Figure 19.
Comparison of the observed (green) and modeled Lyα profiles in RECX-11. The red line corresponds to the profile modeled using the first approach (scaling based on accretion rate and upper envelope of the relation between accretion rate and Lyα luminosity in K. France et al. 2017), while the blue solid line corresponds to the profile modeled using the second approach (scaling based on accretion rate and relation between peak Lyα flux and accretion rate in C. E. Robinson & C. C. Espaillat 2019). The blue dashed line is also generated with the second approach, but the luminosity is multiplied by 4 for BOP checking purposes. The black line is obtained by assuming the same Lyα luminosity as GM Aur.
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