Fig. 6 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. 6.

Power spectra of ﹩\delta _{\mathrm{H}\,\,{}^{{\rm{\small I}}}}+\delta _{\mathrm{DM}\,}﹩ (circles) and ﹩\delta _{\mathrm{H}\,\,{}^{{\rm{\small I}}}}-\delta _{\mathrm{DM}\,}﹩ (squares) of the 12 Mpc box hydrodynamic simulation samples. The physical scale for j is ﹩\Delta v=2^{13-j}\times 4﹩ km s⁻¹. For clarity, the power spectrum of ﹩\delta _{\mathrm{H}\,\,{}^{{\rm{\small I}}}}-\delta _{\mathrm{DM}\,}﹩ is shifted slightly.

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