Fig. 6
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Selection of emission lines that have a NC. The light blue spectrum is ES 22.5. The dark blue spectra are the template that best fits the stellar spectrum (Sec. 3), veiled to match the depth of the photo-spheric lines. The photospheric subtracted spectra are shown in black, with Gaussian best fits superposed in red. The red label specifies the multiple Gaussian model used (Appendix B).
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