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ELUCID. VII. Using Constrained Hydro Simulations to Explore the Gas Component of the Cosmic Web

  • Authors: Renjie Li, Huiyuan Wang, H. J. Mo, Shuiyao Huang, Neal Katz, Xiong Luo, Weiguang Cui, Hao Li, Xiaohu Yang, Ning Jiang, Yuning Zhang

Renjie Li et al 2022 The Astrophysical Journal 936 .

  • Provider: AAS Journals

Caption: Figure 8.

The predicted electron pressure (﹩{P}_{{\rm{e}},\mathrm{pre}}﹩) vs. the simulated electron pressure (﹩{P}_{{\rm{e}},\mathrm{sim}}﹩). The contours enclose, respectively, 10%, 30%, 50%, 70%, 90%, 99% of all the cells, each being a cube of ﹩{(0.1\,{h}^{-1}\mathrm{Mpc})}^{3}﹩. The points show the median ﹩{P}_{{\rm{e}},\mathrm{sim}}﹩ as a function of ﹩{P}_{{\rm{e}},\mathrm{pre}}﹩, and error bars show the 16 and 84 percentiles. The dashed line corresponds to the one-to-one relation between the predicted and simulated electron pressures. Note that a typical filament with ﹩{\rho }_{{\rm{b}}}=10{\bar{\rho }}_{{\rm{b}}}﹩ and ﹩\mathrm{log}(T/{\rm{K}})=5.5﹩ has a pressure of 0.71K cm−3.

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