The MAGPI Survey: Drivers of kinematic asymmetries in the ionised gas of $z\sim0.3$ star-forming galaxies

• DOI: 10.48550/arxiv.2311.10268
• Publication Date: 2023-01-01
• Authors: Bagge, R. S.; Foster, C.; Battisti, A.; Bellstedt, S.; Mun, M.; Harborne, K.; Barsanti, S.; Mendel, T.; Brough, S.; Croom, S. M.; Lagos, C. D. P.; Mukherjee, T.; Peng, Y.; Remus, R-S.; Santucci, G.; Sharda, P.; Thater, S.; van de Sande, J.; Zafar, L. M. Vale...; Ziegler, B.
• Keywords: Astrophysics of Galaxies (astro-ph.GA); FOS: Physical sciences; Astrophysics - Astrophysics of Galaxies

Galaxy gas kinematics are sensitive to the physical processes that contribute to a galaxy's evolution. It is expected that external processes will cause more significant kinematic disturbances in the outer regions, while internal processes will cause more disturbances for the inner regions. Using a subsample of 47 galaxies ($0.27<br/>e.g., 20 pages, 19 figures<br/>