Fig. 6
Comparison of SSe and SSa spectra for the high/low state spectra of V5116 Sgr (top) and the two best examples of SSa, V2491 Cyg, and SSe, U Sco, (bottom). The emission line component in SSe spectra, obtained by removing the weak continuum component, is added the continuum component of an SSa spectrum. The continua are approximated by blackbody models. The SSe emission line components are comparable in strength to complex atmospheric absorption/emission features in SSa.
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