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Fig. 16


Left: model spectrum for Balmer and permitted lines for Nova Mon 2012 for vrad = 4000 km s-1, θo = 5°, θi = 60°, ΔR/R = 0.3, i = 70°. Right: pseudo-image of the ejecta corresponding to the parameters used for the profile simulation (the image is cut at 30% of the peak flux).

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