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

J. A. Weber; A. W. A. Pauldrach; J. S. Knogl; T. L. Hoffmann

doi:10.1051/0004-6361/201220897

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Volume 555 (July 2013)

A&A, 555 (2013) A35

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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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