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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. 7.

Redshift evolution of Δψ in the ﹩\zeta =12﹩ (thin lines) and ﹩\zeta =40﹩ (thick lines) models. The curves are ﹩\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). The redshifts in the two models differ.

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