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The origin of the enhanced metallicity of satellite galaxies

, , , , , , , and . (2016)cite arxiv:1609.03379Comment: 22 pages, 15 figures; accepted by MNRAS.

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Other publications of authors with the same name

The Hydrangea simulations: galaxy formation in and around massive clusters, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1703.10610Comment: 22 pages, 15 figures (18 pages, 14 figures without appendices); submitted to MNRAS.The origin of the enhanced metallicity of satellite galaxies, , , , , , , and . (2016)cite arxiv:1609.03379Comment: 22 pages, 15 figures; accepted by MNRAS.LoCuSS: Pre-processing in galaxy groups falling into massive galaxy clusters at z=0.2, , , , , and . (2017)cite arxiv:1710.04230Comment: 5 pages, 2 figures. Accepted for publication in MNRAS Letters.Overconsumption, outflows and the quenching of satellite galaxies, , and . (2014)cite arxiv:1404.6251Comment: Resubmitted to MNRAS Letters, 6 pages, 2 figures.The stellar mass function and efficiency of galaxy formation with a varying initial mass function, , and . (2013)cite arxiv:1311.5230Comment: 17 pages, 10 figures. Submitted to MNRAS.Do group dynamics play a role in the evolution of member galaxies?, , , , , , , , , and 1 other author(s). (2013)cite arxiv:1308.1406Comment: 14 pages, 6 figures, MNRAS accepted.