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Idealized models for galactic disk formation and evolution in 'realistic' LambdaCDM haloes

, and . (2012)cite arxiv:1203.1190Comment: 24 pages, 20 figures, submitted to MNRAS.

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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.Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way, and . (2020)cite arxiv:2012.07846Comment: submitted to MNRAS.The host galaxies of active galactic nuclei, , , , , , , , , and 3 other author(s). Monthly Notices of the Royal Astronomical Society, 346 (4): 1055--1077 (2003)Fitting the universe on a supercomputer., and . Comput. Sci. Eng., 1 (2): 36-45 (1999)Universality in the structure of dark matter haloes over twenty orders of magnitude in halo mass, , , , , , and . (2019)cite arxiv:1911.09720Comment: 35 pages, 8 figures, submitted.A Universal Density Profile from Hierarchical Clustering, , and . (1996)cite arxiv:astro-ph/9611107 Comment: typos in eqs A5 and A14 corrected. In press in the ApJ, Dec 1, 1997. Full PS file with figures can be obtained from http://penedes.as.arizona.edu/~jfn/preprints/dprof.ps.gz.The Origin of Disks and Spheroids in Simulated Galaxies, , , , , , , and . (2011)cite arxiv:1112.2220Comment: 11 pages, 8 figures. Submitted to MNRAS.Simulating the universe., , , , , , , and . PDP, page 234-239. IEEE Computer Society, (1997)Estimating gas masses and dust-to-gas ratios from optical spectroscopy, , , , , and . (2013)cite arxiv:1304.3492Comment: 32 pages, 25 figures. Accepted for MNRAS.The Structure of Cold Dark Matter Halos, , and . (1995)cite arxiv:astro-ph/9508025 Comment: compressed and uuencoded PS file. 22 pages including 14 figures. 447875 bytes. Submitted to ApJ on August 1, 1995.