Fig. 7
Comparison of the spectrum of V4332 Sgr in 2005 (black: this paper) to that observed in 2009 (red: Kamiński et al. 2010). Green: model atmosphere (Teff = 3600 K, log g = 0.5) reddened with EB−V = 0.35 and fitted to the 2009 spectrum. Blue: model atmosphere (Teff = 3300 K, log g = 0.0) reddened with EB−V = 0.35 and fitted to the 2005 spectrum.
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