Fig. 17 from Intermittent Features of the Quasar Lyα Transmitted Flux: Results from Cosmological Hydrodynamic Simulations

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Intermittent Features of the Quasar Lyα Transmitted Flux: Results from Cosmological Hydrodynamic Simulations

Authors: Long-Long Feng, Jesus Pando, and Li-Zhi Fang

Feng, Pando, & Fang 2003 The Astrophysical Journal 587 487.

Provider: AAS Journals

Caption: Fig. 17.

Structure functions ﹩\mathrm{\ln}_{2}[ S^{2n}_{j}/ ( S^{2}_{j}) ] ﹩ vs. j of H I density field ﹩\delta _{\mathrm{H}\,\,{}^{{\rm{\small I}}}}﹩. The physical scale for j is ﹩\Delta v=2^{13-j}\times 4﹩ km s⁻¹.

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