Three-dimensional modeling of ionized gas - I. Did very massive stars of different metallicities drive the second cosmic reionization?

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Fig. 12

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As Fig. 10, but the flux is now shown on a logarithmic scale. On this scale it is verified that the ionizing fluxes shortward of the He ii ionization edge (4 Rydberg) vary considerably along with a change of the metallicity (cf. Table 2).

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