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The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters

, , , , , , , , , , , , , , и . (2022)cite arxiv:2210.10060Comment: 17 pages, 14 figures, submitted to MNRAS, comments welcome.

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Helmuth Frenk

Sonja Frenk

Joachim Frenk

Marina Frenk

Karl Robert Frenkel

 

Другие публикации лиц с тем же именем

Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure, , , и . (2021)cite arxiv:2102.08404Comment: 31 pages, 20 figures; submitted to MNRAS; Comments welcome.Properties of HI discs in the Auriga cosmological simulations, , , , , , и . (2016)cite arxiv:1610.01594Comment: 18 pages, 15 figures, 1 table. Submitted to MNRAS. Computed HI properties available at http://auriga.h-its.org/data.html.Winds of change: reionization by starburst galaxies, , , , , , и . (2016)cite arxiv:1606.08688Comment: 14 pages, 8 figures, submitted to MNRAS, comments welcome.Cosmic cookery: making a stereoscopic 3D animated movie, , , , , , , , и . 6055, стр. 605505--605505-12. (2006)The mass profile and accretion history of cold dark matter haloes, , , , , , , , и . Monthly Notices of the Royal Astronomical Society, 432 (2): 1103--1113 (21.06.2013)The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics, , , , , , , , , и 2 other автор(ы). (2022)cite arxiv:2210.10059Comment: submitted to MNRAS, 23 pages, 19 figures, for future public data release, see https://www.mtng-project.org.The MilleniumTNG Project: The galaxy population at $z8$, , , , , , , , , и 4 other автор(ы). (2022)cite arxiv:2210.10066Comment: 11 pages, 7 figures, Comments welcome -- Part of the initial set of papers introducing the MilleniumTNG project. Visit www.mtng-project.org for more details.The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters, , , , , , , , , и 5 other автор(ы). (2022)cite arxiv:2210.10060Comment: 17 pages, 14 figures, submitted to MNRAS, comments welcome.The effect of baryons on the inner density profiles of rich clusters, , , , , , , , , и . (2014)cite arxiv:1409.8297Comment: 13 pages, 7 figures, submitted to MNRAS.The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end, , , , , , и . (2016)cite arxiv:1607.07445Comment: 15 pages, 8 figures.