Fig. 7.
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Spectral evolution between 1000 Å and 1 μm and from 250 to 3100 d for model he3p30 under the influence of a constant power of 1039 erg s−1. All spectra are normalized to a maximum flux of unity at each epoch. Contributions by species (e.g., those associated with oxygen include contributions from O I, O II, and O III) are indicated with a colored shading.
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