Properties of the diffuse gas component in filaments detected in the Dianoga cosmological simulations

Ilc, Samo (author), Fabjan, Dunja (author), Rasia, Elena (author), Borgani, Stefano (author), Dolag, Klaus (author)

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.

• Language: English
• Keywords: galaxies clusters, intergalactic medium, large-scale structure
• Work type: Article
• Typology: 1.01 - Original Scientific Article
• Organization: FMF - Faculty of Mathematics and Physics
• Publication status: Published
• Publication version: Version of Record
• Year: 2024
• Number of pages: 16 str.
• Numbering: Vol. 690, art. A32
• PID: 20.500.12556/RUL-163142
• UDC: 524.8
• ISSN on article: 1432-0746
• DOI: 10.1051/0004-6361/20245007
• COBISS.SI-ID: 209928707
• Publication date in RUL: 02.10.2024

Record is a part of a journal

• Title: Astronomy & astrophysics
• Shortened title: Astron. astrophys.
• Publisher: EDP Sciences
• ISSN: 1432-0746
• COBISS.SI-ID: 392577

Licences

• License: CC BY 4.0, Creative Commons Attribution 4.0 International
• Link: http://creativecommons.org/licenses/by/4.0/
• Description: This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.

Projects

• Funder: ARIS - Slovenian Research and Innovation Agency
• Project number: P1-0188-2022
• Name: Astrofizika in fizika atmosfere