Fig. 14
Comparison of the flux-normalized infrared spectra of LHA 120-S 35 taken with the OSIRIS (in red solid line) and FLAMINGOS-2 (in dash-dotted black line) spectrographs. Despite of the poor S/N of the OSIRIS data, it can be seen that while the Paβ line is more than twice stronger than in the FLAMINGOS-2 spectrum, the Brackett series emission lines are weaker.
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