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The Growth of H II Regions During Reionization

  • Authors: Steven R. Furlanetto, Matias Zaldarriaga, and Lars Hernquist

Furlanetto, Zaldarriaga, & Hernquist 2004 The Astrophysical Journal 613 1.

  • Provider: AAS Journals

Caption: Fig. 11.

Redshift evolution of Δψ if we assume that each galaxy hosts its individual H II region. All curves assume ﹩\zeta =40﹩. The lines are for ﹩\overline{x}_{\mathrm{H}\,}=0.96﹩ (dotted), ﹩\overline{x}_{\mathrm{H}\,}=0.8﹩ (short‐dashed), ﹩\overline{x}_{\mathrm{H}\,}=0.5﹩ (long‐dashed), and ﹩\overline{x}_{\mathrm{H}\,}=0.26﹩ (solid).

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