Fig. A.1.
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Spectral evolution of models logP2p75, logP2p80, logP2p85, and logP2p90. The CMFGEN time sequences are computed at time steps ti such that ti + 1/ti= 1.1. Here, we show fewer time steps for better visibility so that tiplot + 1/tiplot∼ 1.3. As for Fig. 6, we illustrate the flux associated with He I lines (dark shade) and H I lines (light shade).
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