Autor der Publikation

It's not easy being green: The evolution of galaxy colour in the EAGLE simulation

, , , , , , und . (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.

Bitte wählen Sie eine Person um die Publikation zuzuordnen

Um zwischen Personen mit demselben Namen zu unterscheiden, wird der akademische Grad und der Titel einer wichtigen Publikation angezeigt. Zudem lassen sich über den Button neben dem Namen einige der Person bereits zugeordnete Publikationen anzeigen.

 

Weitere Publikationen von Autoren mit dem selben Namen

The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end, , , , , , und . (2016)cite arxiv:1607.07445Comment: 15 pages, 8 figures.SWIFT: task-based hydrodynamics and gravity for cosmological simulations, , , und . (2015)cite arxiv:1508.00115Comment: Proceedings of the EASC 2015 conference, Edinburgh, UK, April 21-23, 2015.Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations, , , , , , , , , und . (2015)cite arxiv:1504.04374Comment: 20 pages, 7 figures, submitted to MNRAS.The effect of baryons on the inner density profiles of rich clusters, , , , , , , , , und . (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, , , , , , und . (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.A Hybrid MPI+Threads Approach to Particle Group Finding Using Union-Find., , , und . PARCO, Volume 36 von Advances in Parallel Computing, Seite 263-274. IOS Press, (2019)EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies, , , , , , , und . (2022)cite arxiv:2210.09978.A machine learning approach to mapping baryons onto dark matter halos using the EAGLE and C-EAGLE simulations, , , , , , und . (2021)cite arxiv:2106.04980Comment: 15 pages, 13 figures, submitted to MNRAS. Comments welcome!.Swift: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications., , , , , , , , , und 17 andere Autor(en). CoRR, (2023)The Hydrangea simulations: galaxy formation in and around massive clusters, , , , , , , , , und 5 andere Autor(en). (2017)cite arxiv:1703.10610Comment: 22 pages, 15 figures (18 pages, 14 figures without appendices); submitted to MNRAS.