Fig. 12
Comparison between the Hβ (left) and Hα (right) line profiles computed in NLTE with Cloudy employing an incident stellar flux corresponding to a star with an effective temperature of 9600 K (black; Borsa et al. 2019) and 10 200 K (red; Gaudi et al. 2017). To ease the comparison, the range of the y-axis is the same as that of the top panels of Fig. 6.
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