Cosmic metal invaders: Intergalactic O VII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation

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Fig. 10.

Normalised density distribution of the hot WHIM (turquoise line) and O VII (dashed purple line) as a function of distance from the closest halo centre, in units of virial radius, R₂₀₀. As in Fig. 1, haloes were selected within the range of log M₂₀₀(M_⊙) = 12 − 13.5.

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