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Do group dynamics play a role in the evolution of member galaxies?

, , , , , , , , , , и . (2013)cite arxiv:1308.1406Comment: 14 pages, 6 figures, MNRAS accepted.

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David J Lutz

David J Downs

David J Roy

-J David Lin

David J Roy

 

Другие публикации лиц с тем же именем

Metallicity evolution at 0.8 < z < 2.6 from the LUCI, SINS/zC-SINF and KMOS-3D surveys, , , , , , , , , и 26 other автор(ы). (2014)cite arxiv:1405.6590Comment: 7 pages, 3 figures, submitted to ApJL.The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^3D$, , , , , , , , , и 20 other автор(ы). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7, , , , , , , , , и 16 other автор(ы). (2017)cite arxiv:1703.07778Comment: 7 pages, 5 figures, submitted to ApJ Letters.Measures of Galaxy Environment I - What is &quot;Environment&quot;?, , , , , , , , , и 12 other автор(ы). (2011)cite arxiv:1109.6328 Comment: 14 pages, 9 figures, 1 table, accepted to MNRAS.Do group dynamics play a role in the evolution of member galaxies?, , , , , , , , , и 1 other автор(ы). (2013)cite arxiv:1308.1406Comment: 14 pages, 6 figures, MNRAS accepted.The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , и 21 other автор(ы). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOS, , , , , , , , , и 7 other автор(ы). (2015)cite arxiv:1503.08831Comment: 6 pages, 5 figures, accepted for publication in ApJL.