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Disambiguation of "Theuns, Tom"

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Simulating the dark matter decay signal from the Perseus galaxy cluster

, , , , , , and . (2019)cite arxiv:1903.11608Comment: 6 pages and 3 figures, plus 5 pages and 6 figures in supplemental material. Accepted for publication in ApJL.

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Marieta Ioana Toma

Zentrosomenmorphologie in Prostatakarzinomen: eine immunhistologische Studie mit Korrelation zu DNA-Ploidie und kliniko-pathologischen Parametern. TU Dresden, (2008)

Tom Walde

Tom Herrmann

Tom Hellriegel

Tom Nilges

 

Other publications of authors with the same name

How supernova explosions power galactic winds, , and . (2012)cite arxiv:1211.1395Comment: 27 pages, 21 figures, submitted to MNRAS. Additional media at http://astro.dur.ac.uk/~rmdq85/.On the connection between the intergalactic medium and galaxies: The HI-galaxy cross-correlation at z < 1, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1309.5950Comment: 63 pages, 26 figures, 20 tables; To be accepted by MNRAS (reviewed); Comments still welcome.The effect of baryons on the inner density profiles of rich clusters, , , , , , , , , and . (2014)cite arxiv:1409.8297Comment: 13 pages, 7 figures, submitted to MNRAS.The metallicity of galactic winds, , and . (2014)cite arxiv:1410.7391Comment: 19 pages, 15 figures, accepted to MNRAS.Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations, , , , , , , , , and . (2015)cite arxiv:1504.04374Comment: 20 pages, 7 figures, submitted to MNRAS.The broadening of Lyman-alpha forest absorption lines, , and . (2015)cite arxiv:1502.05715Comment: 12 pages, 15 figures, Re-submitted to MNRAS after addressing the referee's comments.It's not easy being green: The evolution of galaxy colour in the EAGLE simulation, , , , , , and . (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, , , , , , and . (2016)cite arxiv:1607.07445Comment: 15 pages, 8 figures.SWIFT: task-based hydrodynamics and gravity for cosmological simulations., , , and . CoRR, (2015)Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure, , , and . (2021)cite arxiv:2102.08404Comment: 31 pages, 20 figures; submitted to MNRAS; Comments welcome.