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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.

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Matthieu Felsinger

Matthieu Hammer

Matthieu Saubanère

Friedrich Matthieu

Matthieu Barukinamwo

 

Другие публикации лиц с тем же именем

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.It's not easy being green: The evolution of galaxy colour in the EAGLE simulation, , , , , , и . (2016)cite arxiv:1601.07907Comment: 15 pages, 10 figures. Submitted to MNRAS. All comments welcome. Larger version of Fig. 1 included in source. For the animated evolution of the EAGLE intrinsic u-r CMD (with central and satellite galaxies coloured red and blue respectively) see http://community.dur.ac.uk/j.w.trayford/media/CMD_evolution_EAGLE.mp4.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.Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations, , , , , , , , , и . (2015)cite arxiv:1504.04374Comment: 20 pages, 7 figures, submitted to MNRAS.EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies, , , , , , , и . (2022)cite arxiv:2210.09978.A machine learning approach to mapping baryons onto dark matter halos using the EAGLE and C-EAGLE simulations, , , , , , и . (2021)cite arxiv:2106.04980Comment: 15 pages, 13 figures, submitted to MNRAS. Comments welcome!.SWIFT: task-based hydrodynamics and gravity for cosmological simulations., , , и . CoRR, (2015)A Hybrid MPI+Threads Approach to Particle Group Finding Using Union-Find., , , и . PARCO, том 36 из Advances in Parallel Computing, стр. 263-274. IOS Press, (2019)The Milky Way's plane of satellites: consistent with $Łambda$CDM, , , , , , , , , и . (2022)cite arxiv:2205.02860.Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations, , , и . (2020)cite arxiv:2012.03974Comment: Submitted to MNRAS. Comments to joshua.borrow@durham.ac.uk.