Fig. 3

Comparison between the N-type spectral standard stars RS Cyg (C-N5.5 C23, red), Z Psc (C-N5 C24, blue), and V460 Cyg (C-N5 C24.5, green) from Barnbaum et al. (1996) with the Hermes spectrum of LX Cyg smoothed to the resolution of the atlas spectra (R = 2500, black). The spectra are scaled to have the same maximum flux in the shown wavelength range. Vertical dotted lines indicate the wavelengths of C2 band heads from the Swan system (Kipper 2004).
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