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Properties of the diffuse gas component in filaments detected in the Dianoga cosmological simulations
Samo Ilc, Dunja Fabjan, Elena Rasia, Stefano Borgani, Klaus Dolag
Izvirni znanstveni članek
Oznake: galaxies clusters;intergalactic medium;large-scale structure;
Context. Cosmic filaments are observationally hard to detect. However, hydrodynamical cosmological simulations are ideal laboratories where the evolution of the cosmic web can be studied, and they allow for easier insight into the nature of the filaments. Aims. We investigate how the intrinsic prope ...
Leto: 2024 Vir: Fakulteta za matematiko in fiziko (UL FMF)
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