Fig. 6.
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Spectral evolution for models rs100/v1e4/b0p04 (left) and rs10/v1e4/b0p04 (right). Although the time step adopted in our CMFGEN simulations is 10% of the current time, we show spectra here with an increment of about 30% of the current time (i.e., epochs shown are 1, 1.3, 1.8 d etc.). At each epoch, the spectra are normalized to a maximum flux of unity.
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