20.500.12556/RUL-163142 Properties of the diffuse gas component in filaments detected in the Dianoga cosmological simulations 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 properties of filaments are evolving in areas extracted from a larger cosmological simulation. We aim to identify significant trends in the properties of the warm-hot intergalactic medium (WHIM) and suggest possible explanations. galaxies clusters intergalactic medium large-scale structure true false true Angleški jezik Ni določen Članek v reviji 2024-10-02 15:09:13 2024-10-02 15:09:14 2024-10-07 03:39:45 0000-00-00 00:00:00 2024 0 0 16 str. art. A32 Vol. 690 2024 0000-00-00 Zaloznikova Objavljeno NiDoloceno 0000-00-00 0000-00-00 0000-00-00 524.8 1432-0746 10.1051/0004-6361/20245007 209928707 aa50072-24.pdf aa50072-24.pdf 1 C0DBB64D376B220DF84CB980A0667E0D ed48807606aa57ca190b4e0bfd36a155e8b30076e06c6065a89af73e4d1d98b2 e2b9562a-80c0-11ef-b232-0050569b8976 https://repozitorij.uni-lj.si/Dokument.php?lang=slv&id=192650 https://www.aanda.org/articles/aa/pdf/2024/10/aa50072-24.pdf 1 5e30dc39-80bf-11ef-b232-0050569b8976 https://repozitorij.uni-lj.si/Dokument.php?lang=slv&id=192648 Fakulteta za matematiko in fiziko 0 0 0