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The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG

, , , , , , , , , , and . (2017)cite arxiv:1712.00016Comment: Submitted to MNRAS. For an interactive OVI/OVIII visualization, see the 2D explorer at http://www.tng-project.org.

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The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1712.00016Comment: Submitted to MNRAS. For an interactive OVI/OVIII visualization, see the 2D explorer at http://www.tng-project.org.Galactic winds driven by isotropic and anisotropic cosmic ray diffusion in disk galaxies, , , and . (2016)cite arxiv:1605.00643Comment: 6 pages, 5 figures, submitted to ApJL, comments welcome.Resolving small-scale cold circumgalactic gas in TNG50, , , , , , , , and . (2020)cite arxiv:2005.09654Comment: MNRAS submitted, comments welcome.The large-scale properties of simulated cosmic magnetic fields, , , and . (May 29, 2015)The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters, , , , , , , , , and 5 other author(s). (2022)cite arxiv:2210.10060Comment: 17 pages, 14 figures, submitted to MNRAS, comments welcome.The formation of disc galaxies in high resolution moving-mesh cosmological simulations, , and . (2013)cite arxiv:1305.5360Comment: 27 pages, 21 figures, 2 tables. Submitted to MNRAS.Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation, , , and . (2014)cite arxiv:1403.4934Comment: 16 pages, 10 figures, submitted to MNRAS.