Fig. 6.

CO and Brackett γ equivalent widths for all stars. Stars with early-type lines are confirmed with visual inspection of the spectra. In the top panel the stars with an S/N < 20 are shown; in the bottom panel the stars with an S/N > 20 are shown. This S/N is the approximately border of the nearly complete regime of spectral classification. The lines divide absorption (negative) and emission.
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